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Component B has possible invisible companion, period 6.9y. Amp. 0.066V, 1.0819d. V640 CasCPM. 6.09 - 6.14V. CPM. ADS 89B, 11 - >14v. SB1. Blue companion? Giant eclipsing binary. Amp. =>0.2V. Period close to SB. Also classified as ellipsoidal var. AP PscAlpheratz represents the head of [X/Andromeda]. It is approximately 100 [G/light year]s distant and 160 times more [G/luminous] than our [G/Sun]. Alpha CV 2.02 - 2.06V, 0.9636 or 0.966222d. Some spectral lines vary same period, others half period, some nonvariable. ALPHERATZAmp. 0.07V. 6.6 A6IV, 6.9 A8IV, 456y, a = 0.924". Combined mag. and colors. Delta Sct, amp. 0.03V, 0.10101d. CaphCombined mag., color. Primary F4III, comp. B, F3III. Companion 9.44V, +0.34(B-V), -0.14(U-B), G5Ve. Suspected occultation double. AB, CPM, combined mag., color. Component B, 8.2 F3/5 IV, HD 662. C, 14v at 20". Beta C 2.80 - 2.87V, 0.1517495d. ALGENIBAB 6.7 G3III, 7.5 F2IV, 368y, a = 0.564". ADS 161C, 10.37V, K0, at 18", physical. 4.78 - 4.86V. CPM. Lb? 5.06 - 5.16V. AD CetLb 4.26 - 4.46V. AE CetComponent A is SB. ADS 191B, 7.3v dA7 at 12". Period apsidal motion, 3y. Possible radio binary. Ell 6.0 - 6.03V, 0.841678d. UU Psc6.8 B8V, 7.1 B9V, 1600y, a = 1.260". Combined mag., colors. CPM. Fixed sep. 6.47 - 6.52V. EB 5.96 - 6.11B, 6.07 - 6.24V, O9III+O9III, 3.523487d. Spontaneous var. in period. Polarization indicates circumstellar envelope possibly related to mass exchange. AO CasDelta Sct?, 4.49 - 4.55V. CPM. Companion F3V. ADS 254B, 9.5 - 12v. Component B, 12.87v at 63", optical. 3.46 - 3.56V. Deneb Kaitos SheB9.5, A2. SRc 5.0 - 6.9v, 6.6 - 7.7p, 158.9d. T CetOptical. BY Dra, amp. 0.032V, 0.037B, 7.655d. BE CetADS 328B, 8.0 at 0.2". However, ADS 328 appeared single in 1953. ADS 328A, E?, 5.56 - 5.62V. Amp. 0.07V. Suspected double probably single. 2.75 - 2.81V. A* 2.38 K0III, 10.538y, a = 0.072". ANKAAAmp. 0.36V. SR 4.65 - 5.42V, 49d, replaced by cycles 70 - 85d. TV PscLb 4.7 - 4.90V. 7.2 G1V, 7.2 G1V, 5.625y, a = 0.134". Combined mag. and colors. ADS 412AB, CPM. ADS 409B 13.3v at 3" CPM with A. Delta Sct 5.18 - 5.22V, 0.0689797d. GN AndOptical. Delta Sct? Amp. 0.04y, 0.174?d. BB Phe5.5 B7.5V, 5.8 B8.5V, 640y, a = 0.586". Combined mag. and colors. Components 14 and 13 solar masses. Optical. CPM with HR 127 of which both are close binaries. Also CPM with HR 136. Faint companion at 14". CD 4.9 A2V, 5.6 A7V, 44.43y, a = 0.385". Combined mag., colors. D-C = 1.17V. Alpha Cyg, 4.22 - 4.30B, 0.09028d. ADS 449A is triple occultation system, 6.2, 6.9v, sep. 0.031"; third component 8.8v at 0.196". ADS 449B, 9.7v at 27.5". AB are CPM. Suspect eclipsing because invisible at time of occultation. ADS 455AB, CPM. B, 10.4v K0V. C, 12.3v at 60". Short period binary. Both components A-type. Sep. 0.099". CPM with HR 126 and 127. Delta Sct 6.06 - 6.15V, 0.04931 and 0.0604d. AB 5.6 F7V, 6.3 G0V, 6.92y, a = 0.23". Combined mag., colors, spectrum. ADS 490A?, Delta Sct?, 5.18 - 5.22V. Amp. 0.06B. Delta Sct, 43.0 minutes. BG Cet3.59 - 3.68V. AB 103000?y. Component B spectrum A6V or Am(A3/F0/F2), RV +11.9k/s. Component C, 11.4v, F3 at 55" optical. Beta CMa, amp. 0.035V, 0.096d. Different cycles show different amplitudes, from 0.002 to 0.036V. Doubt has been expressed that this is due to interference between different periods. RV also shows amplitude changing from a few to 25k/s. Line profiles also vary. AG Psc6.3 G7V, 6.4 G8V, 25.00y, a = 0.670". Combined mag., colors. Companion optical. AB CPM. Component C, 15.2v at 48" optical. 5.83 - 5.89V. Binary. D is 8.5v K2IV-V, vsini <54k/s. All components probably optical. Cst 2.20 - 2.27V. SHEDIRCst 6.68V. Z SclSuspected visual double is probably single. Resolved by speckle interferometry 1983.93, sep. 0.145", but unresolved 1981.68, 1983.94. CPM. Alpha C, 5.69 - 5.78V, 3.952d. A0, A9. Diphda is a slightly reddish star a little over 50 [G/light year]s away. It is approximately 40 times more [G/luminous] than our [G/Sun]. 1.96 - 2.11V. DIPHDAHigh velocity star, possible runaway. Physical pair. ADS 624A, EA 5.71 - 6.12B, 4.467224d, i 87.95d. Amp. of primary 0.40V, secondary 0.12V. YZ CasCPM. Companion F8. Gamma Cas, 4.50 - 4.62V, amp. 0.3:R, 1.1679d. AB CPM. Primary F5III, secondary F6IV. Lb?, 5.32 - 5.45V. Delta Sct? 5.99 - 6.03V, 0.1040d. XX PscAB CPM. Companions probably optical. Component A of visual system, EB 3.92 - 4.14V, 17.7695d. AB 3.45 G3V, 7.51 K4Ve, 480y, a = 11.994". Combined mag., colors. Component B, vsini =<25k/s. Companions C-H optical. A possible invisible companion with period about 40y. Component B, 7.51V, +1.39(B-V), +1.03(U-B). AchirdThe two companions probably optical. CPM. CPM with HR 230. 5.33 - 5.39V. Alpha CV 6.10 - 6.14V, 2.156d. Also var. K-line, same period. GO And5.15 - 5.24V. 6.04 - 6.11V. Delta Sct 6.34 - 6.37V, 0.1360d; sinusoidal components 0.0526 and 0.0396d. V526 CasDelta Sct 5.20 - 5.25V, 0.055d. AZ PheDelta Sct 5.17 - 5.27V, 0.110d. Optical. Combined mag. and color. Fixed sep. AB CPM. Component B, dG4. Primary F4IV, secondary G0V. AB optical. AB 6.23 A1V, 6.89 A4V, 360.4y, a = 0.700". Combined mag., colors. Lb? 5.60 - 5.80V. BQ TucAB 6.02 G6IV, 6.41 K6IV, 164.68y, a = 1.014". Resolved by speckle interferometry 1983.94, sep. 0.68". Combined mag., colors. AB CPM. IRAS observations confirm IR excess and yield simple blackbody temperature of 6750 +/- 100K. ADS 782A, Gamma Cas 1.6 - 3.0v. Spectrum and color vary. Expanding circumstellar shell. High-velocity variable mass loss. Variable hydrogen emission, 0.7d. Variable SiIV, CIV, polarization. Variable X-ray source. H alpha indicates rotating disk-like envelope. AB 6.0 B8V, 6.6 B9V, 83.4y, a = 0.252". Total mass, 6 solar. Primary is a mercury-manganese star. All components optical. ADS 805, 790y. Possible periodicities: 19.4, 16.7, 0.95, 0.49d. Visual binary with HR 282. Color for blended images. Lb 5.95 - 6.12V. WW Psc6.7 A3n, 8.0, 450y, a = 0.816". Suspected occultation double, 5.2, 5.2v, sep. 0.25". AB binary. Component B, G8V. Amp. 0.10V. CC TucVisual pair optical. CPM with HR 311. Third component optical. CPM with HR 310. CPM with HR 314. Faint companions probably optical. CPM with HR 313. AB optical. A* 5.15 G5Vp, 21.43y, a = 0.186", mag. diff 2V, sep. 1.4". Subdwarf with five visual and one astrometric components. MarfakMag. and color blend of close pair 4.2, 4.2v. C, 11.5v at 57". Companions probably optical. Delta Sct? 5.8 A2IV, 6.2 A4IV, 28.5y, a = 0.209". Combined mag., colors. Dheneb4.6 B6IV, 5.5 B9V, 371.6y, a = 0.447". Combined mag., colors. Masses 16 and 10 solar. Resolved by speckle interferometry 1983.93, sep. 0.64". Suspected visual double is probably single. MIRACHAB 4.2, 7.0v close binary; vsini of B 87k/s. C, 7.0 F7V at 6.6" CPM. Primary component of visual system. EA 3.92 - 4.42V, 1.6697664d, i 84.7d. Delta Sct? MarfakCst? 5.50 - 5.60V. RU CasL?, 7.1 - 9.0p. Unresolved by speckle interferometry: probably single. AB CPM. Component B, 10.25V, +0.79(B-V), +0.29(U-B), G1V. Delta Sct? 5.93 - 5.98V, 0.05d. AI SclB CPM, 9.11V, +0.92(B-V), +0.25(U-B). CPM with HR 362 at 24". ADS 996A is close occultation double, 6.3, 6.3v, 0.05":. Component B, HR 362 is SB; C, 12.2 is 1" from B. CPM with HR 361. SRb?, amp. 0.15V. Alpha CV?, 5.94 - 5.98V. Mag. 7.38V and colors from Nicolet. However, HD gives 6.38ptm, 7.38ptg. Abt and Biggs RV Bibliography quotes 6.20V; and AGK3 has 7.7ptg. CPM. Component B, G7V. Component C is faint diffuse nebula, NGC 450. RS, 5.35 - 5.58V. AY CetQuadruple system consisting of two close CPM pairs separated by 320": CPD -69d45, components AB, 5.1, 7.3, 5" and CPD -69d44, components CD. AB, 1222.4y, a = 7.64"; CD 7.8 G5, 8.2, 86.2y, a = 1.12". ADS 1073, quintuple system: A = NGC 457 #136; B, 12.3v at 49"; C = NGC 457 #131 = HD 7902, 6.99V, +0.42(B-V), -0.38(U-B), B5Ia at 134", vsini =<25k/s; D, 10.19V, +0.29(B-V), -0.47(U-B) at 179"; E, 10.63V, +0.28(B-V), -0.52(U-B) at 170". BC 7.4, 7.6, 21.5y, a = 0.136". Combined spectrum A1V. AdhilAB 7.1, 7.3v, binary, combined mag. and color. Components C, 12.8v at 46" and D, 10.50v at 249" probably optical. CPM. ADS 1129B, 13.5v, 3" CPM with A. Component C optical, 9.18V, +0.66 (B-V), +0.34(U-B), Am. Delta Sct 6.20 - 6.22V, 0.070d. AV CetProbably optical. Unresolved by speckle interferometry 1981.69. EA? 2.68 - 2.76V, 759d. Ruchbah6.6 F3V, 6.8 F4V, 16.14y, a = 0.1884". Combined mag. and color. AB binary, B 11.7v at 2"; CD 10.4, 10.4 sep. 4.9" at 120" from A. Optical. Binary. Companion 9.38V, +0.19(B-V), +0.00(U-B), A8V, vsini 48k/s. CPM. SRb 9.1 - 12.8p, 370d. R SclA* 2.0 var. F8Ib, 30.46y, a = 0.038". AB physical; B, 8.20V, +0.49(B-V), +0.16(U-B), F3V, 0.0 color excess, vsini =<60k/s; C, 13v at 43"; D, 14v at 83". Polaris is the star currently aligned with Earth's north [G/Celestial Pole]. It is only the 49th brightest star in the sky. Polaris is actually a double star system, made up of two faint stars that are 465 [G/light year]s away. CDelta 1.92 - 2.07V, 3.969778d. Period increases 53 sec./century. Probably unreddened. POLARISCPM. Component B is BD+7d214, 8.02V, +0.53(B-V), +0.06(U-B), G0. 3.39 - 3.49V. Delta Sct 6.56 - 6.59V, 0.090d. WZ SclDelta Sct 5.90 - 5.92V, 0.131d. VX PscAmp. 0.15V. AW PheCPM. Primary K3.5IIIab, secondary G2V. CPM. ADS 1199B, 8.0 - 11.5v? Unresolved by speckle interferometry 1983.94. Probably optical. Amp. about 0.015u, <0.01v, 0.694d. Alpha CV, amp. 0.012V, 0.6684d. Also long-period variations. KK Andbrightening at rate of about 0.045m/100d. OP AndBoth visual companions probably optical. 6.0 F3V, 7.1, probably combined mag. and color. Alpha CV 6.27 - 6.41V, 36.5d; Sp. and magnetic field var., 22-24y. UII and PmII lines vary in 6.7 hrs. GY And6.8 F5, 7.2, 28.3y, a = 0.19". Possible radio binary. Visual companion optical. Achernar is hot, blue giant star that ranks as the 9th brightest star in the sky. It is approximately 125 [G/light year]s distant and 650 times more [G/luminous] than our [G/Sun]. EB or Ell, amp. 0.02V. H alpha var. emission and possible high-velocity mass loss. Expanding circumstellar shell. ACHERNARCPM. Component B, 11.53V, +0.65(B-V), +0.04(U-B). Alpha CV, 5.55 - 5.64V, 3.1848d. V557 CasCPM. Combined mag., colors. Primary F4IV-V, secondary F8V. EA, amp. 0.3V, 16.77d. Third component mag. diff 4.74v, 110" from A. Component B is K2V, optical. Astrometric binary 20y, a 0.12", mag. diff 3-4v. Companion 25% solar mass. AB CPM; B is F2III; C optical. Binary with HR 487, q.v. Gamma Cas 4.03 - 4.11V, 19.5d. Amp. varies in per. 127d. Possible mass loss. Expanding circumstellar shell. 6.4 A2, 7.8 F0, 573.52y, a = 1.07". Torcularis SepteComponent A, astrometric binary unresolved by speckle interferometry. AB 5.4 F1V, 8.6 G9V, 1192.2y, a = 4.652". C 15.0v at 15", D 11.5v at 142". Spectrum of secondary also classified K1V. Delta Sct 6.54 - 6.59V, about 0.2d. VY PscCPM. Component C 8.4v at 21", D 10.2v at 137". Binary. Component B 7.3v A6V, P.A. 166d; RV, 1.8k/s, variable. Confusion in literature as to which component is HD 11154, which 11155. Probably combined mag. and color. CPM. Companion, dG1 is HD 11131. E? 5.46 - 5.68y. V436 PerSecond visual component optical. Baten KaitosDelta Sct, 5.90 - 5.94V, 0.037312d; also possibly 0.1662, 0.038351 and 0.043013d. BD PheVisual companions probably optical. MetallahBinary with HR 546, q.v. Combined mag. HR 545/6, 3.88V; colors also combined. Sp. var. 38 min. Delta Sct, 5.73 - 5.81V, 0.090336d; also possibly 0.1996 or 0.1663d and 0.09417 or 0.10396d. BK CetDelta Sct? SharatanSR 4.3 - 4.5V, 30d. ADS 1534B not CPM with HR 557, component A. ADS 1534AP, CPM, 11.9v at 18". EA? 6.42 - 6.84p, 47.9?d. RR Ari6.76 F7, 6.76 G0, 170.3y, a = 1.05". Alternate orbit 158.4y, a = 1.00". Masses 1.34 and 1.29 solar. Combined mag. and colors. 6.00 - 6.30V. CPM. Optical. ADS 1563B, 7.40V, +0.58(B-V), +0.07(U-B), dG1, CPM; vsini =<25k/s. ADS 1563B; Cst? 7.30 - 740V. Eta2 HyiAB 4.71 A4V, 6.41 F2V, 60.44y, a = 0.653". Perturbation periods of 26 or 39y suspected. C, 13.6v, 24" CPM; D, 13.0v 48" optical. Additional unseen companion suspected. ADS 1598B. B-A varies 1.5 - 3.0v. ADS 1582AB, 8.5, 11.0v, sep. 2.3" at 188" from the bright component D. C, 9.2v at 31" from A. SR? 5.40 - 5.61V. AR CetADS 1625AB, CPM. Binary with HR 596, q.v. Alpha CV? ADS 1621. Uncertain which component varies. B-A from 4.5 - 6.0v. CPM with HR 604. ALMAAKAB 5.90 F8IV, 7.27 F9V, 288.0y, a = 1.256"; or 309.03y, a = 1.34". Other published periods have ranged from 247 to 925y. Combined mag., colors. Suspected occultation double. ADS 1634AB CPM. B, G5V; C at 83" optical. Alpha CV?, 4.68 - 4.73V, 1.89d. SR 6.20 - 6.38V, about 20d. WZ PscHamal, the brightest star in [X/Aries], lies 67 [G/light year]s away and is 70 times more [G/luminous] than our [G/Sun]. HAMALAmp. 0.065V. Sp. var., H alpha profile var. V472 PerSR?, amp. 0.08V. B, mag. diff 6.9v at 5.6". CPM with HR 629. CPM with HR 628. Resolved by speckle interferometry 1983.93, sep. 0.07". Binary. Companion F6V. Amp. 0.075V pulsating? TZ TriPossible nearby star on basis of spectroscopic parallax. 6.6 F3V, 7.08 F6V, 144.7y, a = 0.908". Combined mag., colors. Suspected occultation double, sep. 0.012". E?, 4.35 - 4.38V. AB binary; B, dG4; C, 11.5v at 173". 19.35y, a 0.17" or 18.614y, e 0.616, a 0.158", 10.82AU, i 130.1d. Alternate orbit 19.35y, a = 0.17". Speckle interferometric sep. 0.17", 1983.93. Possible nearby star on basis of spectroscopic parallax. Probably optical. 5.52 - 5.58V. Companion G2V? Mira is a pulsating, variable, red giant star which changes in brightness from [G/magnitude] 3 to magnitude 9 over the course of 331 days. It is approximately 135 [G/light year]s distant. AP var. M7IIIe, var. dBe, 400y, a = 0.85". The faint companion was first predicted in 1920 by Joy on the basis of a slightly displaced blue secondary spectrum. First seen by Aitken in 1923. Visible only when Mira is faint. Light variations on scale of hours superimposed by variations of 10-15 min. and rare flares of 2 min. duration. Components B, 13v at 73" and C, optical. Two variables: Mira and VZ Cet. Mira, ADS 1778A, M 2.0 - 10.1v, 331.96d; var. CO emission from circumstellar envelope. Speckle interferometry indicates large abrupt variation of diameter as a function of wavelength. Hydrogen lines vary on time scale of 1-2 days. Mira was discovered to be variable by Fabricius in 1596, the first such variable discovered. ADS 1778P, Ne "Novoides" class, VZ Cet, 9.5 - 12.0v, dBe. MIRAAmp. 0.05U, 1.31d. Fixed. Amp. 0.05V. Sp. and H alpha profile var. V474 PerCDelta, amp. 0.123V, 7.572d. V440 PerAmp. at 0.58 micrometers about 0.15m. AB 4.64 A3Vp, 6.89 F5, 840y, a = 2.27". A* 4.64 A5p, 52.4y, a = 0.113". Unresolved by speckle interferometry. ABxC 4.51 A5p, 8.40 G7V, probably physical, 6.706" periastron for parabolic orbit. vsini of C =<50k/s. ADS 1860A, Alpha CV, 4.45 - 4.53V, 1.74050d. Also magnetic and Sp. period. AB CPM. Alpha CV 5.71 - 5.88V, 2.997814d. Irregular magnetic var., 15.9d. AB CetCompanion A3IV. ADS 1878A, spectrum variable, shell star. Amp. 0.11V, 0.09R. TZ HorADS 1904AB binary; B, 11v. Suspected occultation double. Delta Sct 6.11 - 6.15V, 0.080d. UU AriDelta Sct? 6.49 - 6.51V, 0.05d, pulsating. TY ForCompanions optical. Companion 7.83V, +0.20(B-V), +0.15(U-B), A7V or A3Vm; vsini 167k/s. Probably optical. Companion, A5, optical. Lb?, 5.39 - 5.53V. Optical. Visual companion 11.7v dM6 at 165", CPM. A* 5.84 K3V, 60y, a = 0.257".. Mass of invisible companion 0.12 solar. Companion at 2" probably about 5v fainter. Unresolved by speckle interferometry. Binary. Companion 9.08V, +0.56(B-V), +0.19(U-B), F7V. Proper motion from AGK3. Earlier McCormick determination, +.022",-.013". M 5.4 - 12.6v, 266.43d. R TriSep. 0.021". CPM with HR 765. HR 764 formerly misidentified as the SB = HR 765. Data for HR 764 and 765 have frequently been interchanged. CPM with HR 764. B 12v, 8" optical; AC CPM; D, mag. diff 5.97v at 40" from A. Beta C 4.05 - 4.10V, 0.16113668d. Per. changed 1965, then increased about 0.7 sec./century. 5.6 F6V, 5.6 F6V, 2.67y, a = 0.108". Combined mag., colors. CPM. Optical. 0.906y, a = 0.057". ADS 2046. Delta Sct?. Uncertain which component varies. AB fixed. AB 6.2, 12.2v, 19" about 6y. Occultations indicate A is triple system, 7.0v A1, at 0.06", and 8.0v at 0.2". Aa resolved by speckle interferometry, sep. 0.045" 1981.68, 0.040" 1981.69. Delta Sct? AB 4.13 F7V, 9.87 M1V, 2720y, a = 22.289". C probably optical. AB CPM. AB binary, combined mag., colors. CPM with BD+2d418, 10.2v M6 at 840". KaffaljidhmaDelta Sct 5.18 - 5.22V, 0.0355d with overtones of 0.046 and 0.061d. UV AriOccultation binary. Combined mag., color. Delta Sct? Binary. Combined mag., color. EA 6.18 - 7.72V, 1.1952473d. Period varies irregularly. i 82.14d. May have two dark companions with orbital periods 23 and 105y. RZ CasAB binary. 7.1 F5, 7.1 F8, 28.5y, a = 0.279". Amp. 0.038V. V480 PerSuspected occultation double, 6.8, 6.8v, sep. 0.2". CDelta 5.78 - 6.16V, 1.949319d, possibly changing. RV varies in same period. SU CasAlpha CV, 5.82 - 5.89V. VZ AriSRb 7.0 - 8.63p, 80d. Secondary cycle 746d. Z EriComponent B, B9V, CPM, vsini 149k/s. Miram in BecvarAB CPM. B 8.8v, A0Vp at 3.2", RV -21k/s, probably optical; C 10.72V, +0.60(B-V), +0.60(U-B), F8V at 25". A is close SB pair with computed sep. 0.00004". Optical system. Delta Sct? AB CPM, B, 13v at 12"; C, optical. AB, 7.2, 9.2v sep. 0.2" possibly optical; AC binary. Primary G6III, secondary G4V. AngetenarA* 4.06 G4III+A4V, 4.150y, a = 0.050". Speckle interferometric sep. 0.080" 1981.67. Circumstellar material surrounding the pair? Visual companions 10.7v at 51" possibly physical; 11.8v at 4" possibly optical. EA, 3.94 - 4.07V. AB 5.9 F4V, 6.5 F6V, 31.37y, a = 0.258". Nearly equal components, 3.7, 4.3 solar. Component C, 9.7v at 14", CPM? Delta Sct? Component B, 15v, possibly spurious. SRb 5.62 - 6.01V, 30d. Rho1 Fl 44M 4.7 - 14.3v, 401.5d, JD2412800-28900; later 407.6d. R HorAlpha CV 5.03 - 5.14V, 2.88422d, same for RV and line-intensities. Also var. magnetic field and H-lines. Rotating spotted star. LT PerAzhaGorgonea SecundaBinary. Companion F7IV. Binary with HR 888. Mag. and colors for combined light. Uncertain if HR 887 or 888 is the variable suspect. CPM with HR 891. CPM with HR 890. MenkarBinary with HR 898. Uncertain which component var. Combined mag. HR 897/8, 2.91V; combined colors, +0.125(B-V), +0.13(U-B). ACAMARLb? 6.11 - 6.29V. CV EriADS 2348B probably optical. Lb? 2.45 - 2.54V. Spectrum var. MENKARSKYLAB observations indicate cool star with hot companion. Components Aa, 14.65y, a = 0.159". Physical nature of B, 11m at 57", uncertain. Close to error box of X-ray source 3U0305+53. CPM. ADS 2312B, 8.5 - 11.0v. SRb 3.30 - 4.0V, about 50d with possibly slow var. in mean brightness in 1100d period. Gorgonea TertiaSee HR 927. Algol is an eclipsing variable star, meaning the light from this star appears to brighten and fade as its companion star passes in front of the star and behind it. The star's [G/magnitude] changes in brightness from mag. 2.1 to mag. 3.4, over the course of 2.8 days. Algol is approximately 100 [G/light year]s distant. A* var. B8V, 1.858y, a = 0.011" or 1.862y, a = 0.104". Apparent apsidal period 28.4y or 32y. Resolved by speckle interferometry: sep. 0.086", 2-3v fainter than primary. This may be Algol C. Four visual companions all optical: B, 12.7v at 59"; C, 12.5 at 67"; D, 10.5 at 82"; BC sep. 15"; E, 12.5v at 11" from D. One of the few known galactic radio sources in which the dominant star is normal. 21cm radio source. ADS 2362A is the prototype Algol star, first discovered as variable by Montanari in 1669. The first period determined by Goodricke in 1783, who also interpreted the variations as due to eclipses. The prototype star proves to be a more a complicated system than most of the Algol-type stars, i.e., compact triple system with separation of the components well under 0.1". The components usually designated Algol A, B, C, sometimes A, a, P. Two formerly additionally desig- nated components D and E, inferred on the basis of an apparent 32 year apsidal motion, are now considered spurious. The various Algol components must not be confused with the visual components ADS 2362 B-E, optical companions at much greater distances from A. ADS 2362A, EA 2.12 - 3.40V, 2.86732442d, abrupt period changes. Orbital and rotation periods synchronized. Rotational velocity 65k/s. Radio flares extending to about 1 A.U., not associated with X-ray activity. Radio flare activity appears correlated with period discontinuities, attributed to "starquakes." Mass flow from K to B8 component at rate of 1.8x10E-08 solar masses/year. Possible circumstellar material associated with radio or H alpha emission. ALGOLSep. 0.03". Runaway star from Ori OB1 association at 59k/s. Presumably originated in Ori 1 assoc. Its space vel. is twice that of HR 1712 = AE Aur and opposite that of HR 2688. These three stars and HR 1996 (Mu Col) appear to be receding from an HII shell of about 110000 solar masses expanding at 10k/s. Beta C 6.10 - 6.23V, 0.15275d. Possibly a SN 4.9 million yrs. ago. UW AriInterferometric double, 6.3, 6.3v. Combined mag. and color. Companion optical. Constant light but large H-line variation. Gorgonea QuartaSuspected occultation double. BoteinSuspected occultation double. SX Ari 5.67 - 5.81V, 0.7278925d. Spectral variations (SiII, HeI, same period). Possible 30 min Sp. var. suggesting star spots related to magnetic field. Silicon abundance varies 10 to 100 times solar, and magnesium 0.03 to 10 times solar. SX AriOptical. Space motion same as for Hyades cluster. AB CPM. C, 13.1v at 11" optical. Delta Sct? CPM. 3.9 F8IV, 6.5 G7V, 314y, a = 4.367". Combined mag., colors. ADS 2402B, 7.0 - 9.03v. FornacisAB 6.8 A2V, 7.3 A4V, 330y, a = 0.386". Combined mag., colors. AB 6.6 G2III, 6.9 A7IV, 44.82y, a = 0.443". Combined mag., colors. Component C 9.5v at 3" physical. Amp. 0.06(U-B). Ell 6.16 - 6.28V, 5.543491d. V423 PerSRb 5.52 - 5.95V, about 158d. TW HorComponent B, 8.0 A7m. CPM. Secondary 8.06V. Amp. 0.02V. Fundamental and overtone periods 0.041 and 0.065d. BN HyiADS 2440. B-A varies from 0.2 to 2.0m. Uncertain which component varies. B6, A1. Zibal in BecvarProbably optical. Gamma Cas, 4.78 - 4.89V. Spectrum var. 4.5y from 1916 to 1931, previously longer cycles, but no changes noted after 1937. R-I also found at -0.03 and -0.05. BK Cam5.6 K1IV, 7.5 G8V, 351.94y, a = 1.077", or 217.20y, a = 0.974". Combined mag., colors. Double discovered by Alvan Clark. CPM with BD-1d474, 9.5v at 11'. ADS 2459B, 7.66V. Doubtful var. Combined light ADS 2459AB, 5.37 - 5.46V. Considered variable by Gould, but never confirmed. CoD-22d1146 C, 11.9v at 251". RW Aur? Amp. 0.10 IR. Binary. AB binary, B is K0V. C, 11v at 40" optical. Lb? 3.57 - 3.72V. Tau4 Eri7.3 - 7.4B. Suspected of being double or triple by Tebbutt in 1893. Components 5.4, 7.9v, sep. 0.15", and 8.4v at 0.67". CPM with HR 1010. Nearby star suspected of variability from discordant photometric observations. CPM with HR 1006. MIRPHAKAB CPM. Binary. AB 6.8 B9V, 7.8 A1V, 259.90y, a = 0.370". Combined mag., colors. H alpha profile var. 7.2, 7.2, sep. 0.1" listed by D. W. Dunham. Probably not occultation double. H alpha profile variable. 550y. AB CPM. Delta Sct. ADS 2552A is close binary, 6.3, 7.7v, sep. 0.010". AB binary; C, 13v at 148". EA, amp. 0.1V, 5.363d. Alpha CV 5.45 - 5.53V, 2.4928d. First helium-weak star found to have periodic variations (1973). V396 PerB CPM, A3V, vsini 100k/s, both components. AB CPM. B, spectral class F2V. Component C, 10.5v at 164". Beta C 6.37 - 6.47V, 0.2101753d, multiple periods, 0.1982, 10.85, 0.01d. KP PerAB 6.8 F3V, 7.6 F9V, 287.7y, a = 1.245". Combined mag., colors. Mass AB, 2.2 solar. C, 10.3v at 92" optical. Ell 5.80 - 5.85V, 0.9171877d. IW PerEll 5.90 - 6.04V, 0.935971d. TU HorAstrometric binary, 25y. Unresolved by speckle interferometry. AB 6.6 A3V, 6.7 A3V, 568.22y, a = 0.650" or 600y, a = 0.719". Combined mag., colors. C, 9.9v at 22" physical. Amp. 0.04V, 0.5d. Hydrogen emission variable. Expanding circumstellar shell. 6.8 F5V, 7.1 F6V, 19.4y, a = 0.225". Combined mag., color. Spectrum variable. 5.88 dG9, 8.83, B-V +0.99, U-B +0.79, K6V, 2101y, a = 8.023". Close radio binary. RS 5.70 - 5.81V, 2.83782d. Min. migrate in period 13y. Brightest of 25 RS CVn binaries known in 1976. Also var. radio emission. Radio flare star with variable polarization. Amp. in red light (6600 A) 0.11 mag. Star spots inferred to be about 1100d cooler than surrounding photosphere. V711 Tau5.23 - 5.32V, amp. 0.11U, 1.93d. EG EriCPM? Position angles disagree by about 40d. Lb 5.04 - 5.17V, 6.7 - 6.85p. BD CamADS 2661A, occultation double?, 7.1, 7.1v, sep. 0.3". Component B, 11.8v at 36" optical. Component D, 8.73V, +0.10(B-V), -0.22(U-B), B8III. Gamma Cas?, 5.55 - 5.58V. Alpha CV? 2.98 - 3.03V, about 1d. Strong variable emission at 1650A, CaII? 5y? Sep. 0.052". vsini of secondary =<50k/s. Binary. Combined mag., colors. Rotational velocity B, 150:k/s. Unresolved by speckle interferometry 1982.16. In interstellar ultraviolet radiation field. Ell 3.79 - 3.85V, 4.419171d, possibly half. AtikRS:, 3.51 - 3.56V, about 10d. Rana in BecvarSuspected occultation binary, sep. 0.0062". Unresolved by speckle interferometry 1981.69. CelaenoCPM. Sep. 0.062". Occultation of 1972 Mar. 19 indicated mag. diff 3.4, sep. 0.010". ElectraPrimary is SB, 4.6, 6.1v, sep. 0.012". Visual pair 4.4, 8.1v, sep. 69". TaygetaSep. 0.003". Unresolved by speckle interferometry 1981.69. Duplicity questioned. Probably cst. Var. helium lines. MaiaAsteropeSuspected occultation double. Sterope IIB possibly optical. Lc 4.35 - 4.48V, amp. 0.12p. BE CamSuspected double probably single star. Variable hydrogen emission. MeropeCPM. Primary K1IIIab, secondary G3IV. Probably optical. Lb? 4.38 - 4.44V. Binary. B-A varies from 2.8 to 4.3V. Uncertain which component varies. Component A is occultation double, sep. 0.031". B, C, D, 8.1 A0V, 8.1 Am(A5/F0/F2) and 8.7v F2V at 117" to 190". Possibly second occultation companion at 0.001", unresolved by speckle interferometry. vsini of B 155k/s. Numerous photometric determinations yield 6.3 for B component. The HD gives 8.1 for 23629 and the IDS indicates 8.1. Burnham, Double Stars, gave 7.0 vis. ALCYONEDelta Sct 5.8 - 5.91V, variable amp. Primary and beat periods, 0.098299 and 0.39206d. V376 Per11.1v companion at 5" noted by Innes not confirmed. Binary. Old disk population runaway star. A variable comparison star was used when HR 1176 was suspected of variablility. A published period, 22.58d, does not satisfy available SB observations, whereas the SB period does satisfy the photometric equally well. However, more observations are badly needed. V467 PerComponent A SB, 4.1, 5.6, sep. 0.006" and 0.019". B, 6.8v at 0.4". AtlasGamma Cas 4.77 - 5.50V. Var. may be clue to shell episodes. Shell ejection 1936 led to decrease in light 1937-1958. Variable hydrogen emission. Shell spectrum shows phase changes every 17 or 34 yrs. Pleione5.81 A3V, 6.21 A5V, 62.28y, a = 0.430". Resolved by speckle interferometry 1983.93, sep. 0.66". Binary with HR 1190. Suspected occultation double. Old disk population runaway star. Amp. 0.06y?, 2.53d. V766 TauCompanion F4V, optical. AB CPM, B 9.16V B8IV; C, 9.12V at 33" optical; D, 10.35V, +0.713(B-V), +0.20(U-B), at 92" optical; E, 9.90V, A2V, +0.33(B-V), +0.17(U-B), at 120" physical. 2.80 - 2.93V. Companion A0, CPM. CPM? Component A possibly optical counterpart or companion of X-ray source 4U0352+30. Possibly a triple system with a neutron star moving around the optical primary in 22.4 hrs., and either apsidal period 581d or close double moving around a distant component in 581d. Rotational velocity of primary, vsini 306k/s. Component ADS 2859B is normal M1III, not T Tau type as once assumed. Space velocities of X Per and Xi Per indicate the two stars approached to within 17 pc 2 million yrs ago. ADS 2859A, Gamma Cas 6.07 - 7.0V, 580.7?d. Amp. about 0.02U. X-ray period 22.4 hrs. Spectrum variable. Sudden decrease in H alpha emission followed by 450 sec. flare in continuum. Possible neutron star companion pulsating in 13.924 min. Simultaneous X-ray and optical obs. 21 Jan. 1975 showed X-ray var. by factor 2 but no corresponding optical 100 sec. quasi periodic photometric var. may indicate binary with compact companion undergoing mass accretion. X PerAB CPM. Component C, 11.4v at 101" optical. P, 12.5v at 279". Binary with HR 1211. Tau8 EriBeta C?, 5.45 - 5.50V. RV possibly var. 0.13169d. Alpha CV 5.97 - 6.00V, 12.4580 or 12.4564d. Rotation and magnetic field same period, no polarity reversal. Spectrum variable, 12.460d. Maximum intensity Eu at minimum light. DO EriAB combined mag. and color. C, 12.7v at 23". AB CPM. B, 7.39V, -0.03(B-V), -0.52(U-B), B9.5V, vsini 300:k/s. Beta C, 2.88 - 3.00V, 0.216:d. Brightest component on visual triple. Photoelectric and spectroscopic resonant periods found are submultiples of 26.9 hrs or 1.12d. V817 TauDelta Sct 6.50 - 6.58V, 0.052d. V386 PerDelta Sct 6.17 - 6.24V, 0.155879d. DL EriDelta Sct. Slightly variable, possibly same period as SB. Menkib5.54 gG8, 6.29 A7, 415.1y, a = 1.00". 2.88 - 2.96V. ZaurakEA 3.3 - 3.80p, B3V+A, 3.952955d, i 86d. Alpha CV 4.62 - 4.67V, 1.2094d. Tau9 EriComponent B, F8V, optical. Third component mag. diff 6.13v, at 100". Lb?, amp. 0.07V. XY DorA is occultation binary, sep. 0.033", unresolved by speckle interferometry 1981.68. Spectrum binary; vsini of early-type component 160k/s. AB, mag. diff 6.5v, sep. 25.5". Beta C amp. 0.04b, over 1d? AB fixed. Some confusion in literature as to which component is A, which B. SZ CAM is Np = B, 6.94V, +0.41(B-V), -0.53(U-B), O9.5V, vsini 160:k/s. Colors of both components have been described as "yellowish" even though both have B-type spectra. Component Q, 10.39V, +0.58(B-V), -0.26(U-B). Two variables: ADS 2984A = NSV 1458, amp. 0.05V, SB; component B = SZ Cam, Np, EA 7.0 - 7.29B, changing period, abrupt change in 1972 from 2.6984378 to 2.69854365, later to 2.6985439d. SZ CamLb? 4.42 - 4.64V, 25d. Alpha CV 5.15 - 5.22V, 7.227424d. Earlier period 11.94d still frequently quoted. Lines of SiII, SrII, possibly TiII var. GS TauGamma Cas 4.00 - 4.10V, 55?d. Slow var. possibly associated with emission spectrum. MX PerCPM with GC 4949 at 12' = ADS 2995, a triple system 7.3 dK2, 9.0 sep. 1"; C at 234". CPM. B is dG8. ADS 2999, B-A varies from 2.95 to 3.55V. Uncertain which component varies. Delta Sct? Primary of ADS 3006 is occultation binary, sep. 0.05". Visual companion, 9.3v at 4.4", CPM. Delta Sct 5.37 - 5.44V, 0.144923d. Possible other periods 0.126535 and 0.126569d. Light curve composite of 0.1449 and 0.1120d. Amp. B-V 0.035, amp. U-B 0.015. Variations in U-B opposite in phase from B-V. IM TauProbably var., amp. 0.08V. Spectrum var. Delta Sct 4.00 - 4.05V, 0.0815d. Secondary per. 0.1291d. BeidA* 4.13 G0Ib, 0.778y, a = 0.019". AB CPM; B, 11.8v at 15". C , 10.25V, +0.47(B-V), +0.06(U-B), B8. ADS 3071A, 4.1 - 4.24V. B, 13.6v at 8"; C, optical. 6.0 F2V, 6.1 F3V, 7.18y, a = 0.135". Resolved by speckle interferometry 1983.93, sep. 0.09". AB binary; C, 12v at 32" optical. AB binary, B is G2V. CPM with HR 1322. BY, 6.92 - 7.00V. The fainter component of ADS 3085. Amp. 0.06V, 6.8d rotational period traced by large scale star-spot activity. V891 TauCPM with HR 1321. 6.28 - 6.37V. V774 TauSource of weak radio emission. Ell 4.59 - 4.65V, 1.527365d. Radio binary showing radio flare activity. Third component may eclipse primary. b PerBC 9.51 A2, 11.18 M4Ve, 252.1y, a = 6.943". Component B is white dwarf. Component A, CPM. ADS 3093C; UV, min. 11.18V, +1.50 (B-V), 12.16 - 13.85U. X-ray source. KeidDuplicity questioned. Visual primary is speckle-interferometric double, sep. 0.076". Visual companion 10.7v at 166". Amp. 0.020V. EW? or Delta Sct? 4.23 - 4.27V, per. between 0.33 and 1.0d. CPM with HR 1341. Optical. CPM with 1339. 0.07V, 1.569d (light and spectrum). V724 TauAmp. 0.3V. Amp. 0.1V. Hyadum IC, 11.8v at 49". Small amp., possible periods 0.96, 1.93, 8.5, 0.89d, with 8.5 slightly favored (Manfroid and Mathys 1985, A&AS, 59, 429). Optical. Astrometric binary unresolved by speckle interferometry. Amp. 0.01V, 7.29?hrs. V469 PerBinary. Delta Sct 5.56 - 5.59V, 0.054d. V483 TauADS 3146B, 10.5 - >12V. Delta Sct 5.20 - 5.26V, 0.036d or double. V696 TauBinary. Combined mag., colors. Amp. 0.015y, 2.833d. TT RetSecondary F7V, vsini 90k/s. BY, amp. 0.12V, 154d. EK EriVaries several hundredths of a mag. on a time scale of days. EM EriCPM. Companion G0V. B, 13.0v at 36" optical. CPM. Component A suspected occultation double; component B, G2V, strong lithium. Amp. 0.1V. Hyadum IIAB 6.6 F1V, 6.9 F3V, 76.92y, a = 0.500". Combined mag., color. Component C, 12v at 37" optical; D, 8.25V, +0.57(B-V), +0.04(U-B), G0 at 45" CPM. Amp. 0.13V. AB CPM. B is A0. Component A suspected occultation double. ADS 3188B, 9.6 - 11.3v. 5.8 A3V, 5.9 A4V, 51.6y, a = 0.18", or 55.40y, a = 0.20". Optical. Delta Sct? Amp. 0.12V. Kappa1 Tau is occultation double. Together with Kappa2 = HR 1388 they form a multiple system of at least 6 components. Delta Sct? See HR 1387. Delta Sct, 5.26 - 5.29V. AB binary; C, 11v at 77" CPM. A blue straggler. Amp. 0.02U, 57.25d. Also magnetic field period. V776 TauAP 7.2 dF5, 7.2, 13.15y, a = 0.133"; occultation binary. Component B, 12.4v at 126". Speckle interferometric sep. of AP 0.093" 1980.94; 0.094" 1983.93. The visual primary is SB, 4.6, 6.5v, sep. 0.020". Component B, 12.5v at 110". Visual primary is occultation double. Component B, 11.1 at 137". V777 TauAB optical? C, 11v at 4" from B. Primary is SB, 6.2, 7.0v, sep. 0.01". Visual secondary is 10.5v at 161", probably optical. Binary. Components G1V and G5V. AB binary; C, 11.32V at 121" optical. Fourth component 13.3v at 17" from C. Sep. 0.024". Ain6.8 A2, 7.0, 175.7y, a = 1.250". CPM with HR 1412. Not clear if there are one or two occultation companions: mag. diff 3.8v, sep. 0.082", another possible mag. diff 8v, sep. 0.2". CPM with HR 1411. Close occultation binary, 3.5, 5.8v, sep. 0.005". Delta Sct, amp. 0.03V (variable), 0.080d. Possibly also eclipsing. The2 TauAB binary. B, 6.94V, +0.16(B-V), -0.70(U-B), B1IV? vsini =<25k/s. Suspected of being double; probably single. 5.7 F0V, 7.98 G2V, 189.5y, a = 1.01" (alternates 180.0y, a = 1.00"; 170y, a = 1.029"). Combined mass 2.82 solar. Speckle interferometric sep. 1.300" (1980.94). Gamma Cas 5.41 - 5.49V. Expanding circumstellar shell; possibly high velocity mass loss. Equivalent width of H alpha variable. DU EriCPM. Component A of visual pair is occultation double 5.6, 5.6v, sep. 0.02"; component B, 6.7v at 250". Delta Sct? SX Ari 5.73 - 5.82y, 1.374d. Var. helium lines. DZ EriBinary. No change after 113y. CPM. Alpha CV, amp. 0.035V, 0.065U, 3.80d. EH EriLb? 5.10 - 5.13V, amp. 0.20p. DV EriA* 4.27 G8II+B, 28.67y, a = 0.054"(not confirmed). Visual duplicity questioned. Unresolved by speckle interferometry 1983.93. Known as the "red eye of the Bull'" Aldebaran is a red giant star, 40 times Larger than our Sun. It is approximately 68 [G/light year]s distant and ranks as the 13th brightest star in the sky. AB binary. B is 13.5v, dM2 at 31". CD, 122" from A is 11.2, 13.6v sep. 2" also binary but independent of AB. Lb 0.75 - 0.95V. Var. H and K emission. ALDEBARANCPM. Companion 7.84V, +0.54(B-V), +0.04(U-B), F8V. vsini =<25k/s. ADS 3317A, E?, 4.23 - 4.30V. CPM. Companion A7V. Component C optical. Beta C 3.4 - 3.60p, 0.17790414d, changing. Probable interference periods 0.1779 and 0.1735d with beat period of 7.0256d. Possibly also E, 103.9d. Theemim3.8 A0IIIp, 4.3 B9IV, 13.00y, a = 0.212". Combined mag., colors. Companion 10v at 78" optical. Alpha CV 3.26 - 3.30V, amp. 0.10u, 2.943d. AB 5.8 F0V, 7.4 F9V, 26.25y, a = 0.18" or 26.797y, a = 0.157". ABxC 5.6, 7.3, 425.0y, a = 1.38". Component D, 13.2v at at 24" optical. Spectral classes component A, A9V; B, F8V; C, F8V. ADS 3359A, Cep?, 5.05 - 5.10V, 5d? 5.3 - 5.38V. Occultation indicated mag. diff 0.37v, sep. 2.117" (half the visual sep.) and PA 78d in contrast to visual 194d. EA 5.92 - 6.7V, 2.056302d, period possibly variable. HU TauIDS gives AB, 5.3, 11.8v sep. 30". Optical. Component C by Wallenquist. Binary with HR 1479 at 431" and with fainter SB companion, 7.4v at 0.0015". Binary with HR 1478. Sceptrum280.0y, e 0.56, a 0.45", i 51.9d, mag. diff 0.0. AB, CPM. Third component by Wallenquist, mag. diff 6.42, sep. 90". B is 11.9 at 34". Uncertain which of components B,C is the brighter: discordant magnitudes. Component A of triple, SRb 4.8 - 6.6v, about 338d. R DorSeen as double only in 1877 and 1923. SRb 4.28 - 4.36V, 30d. DM EriAB CPM, 4.3, 8.9v sep. 0.1", 28y? C, 7.3A1V at 63" vsini 100k/s, physical. D. W. Dunham gives 4.9, 5.6v sep. 0.1" and 4.9, 6.4 sep. 0.0005". CPM. Comp. A of double, Delta Sct? 7.2 G5V, 7.3 G6V, 552.30y, a = 3.164". Combined mag., colors. Both components also classified G3V. CPM with HR 1506. Alpha CV?, amp. 0.025V. DW EriDelta Sct? In Hyades instability strip. Gamma Cas 5.76 - 5.98V. Equivalent width of H alpha is variable. Amp. 0.09R, 0.05(R-I). DX EriVisual companion probably optical. Delta Sct? Amp. 0.05V. Delta Sct 5.09 - 5.11V, 0.042d. V480 TauCPM. SRb 4.65 - 4.88V, about 30d. Companion optical. CPM with HR 1564. B-V for combined light. CPM with HR 1563. Ell 3.66 - 3.73V, 3.700363d. Pi5 OriAB 4.5, 7.8, 284.0y, a = 0.78". C, 11v at 26" CPM, possibly physical. 4.0 - 4.15p. Hassaleh in BecvOptical group. Cst? 5.72V. R Eri136.0y, e 0.32, a 0.425", i 88d, mag. diff 1.0. Component A suspected occultation double. Two visual companions. Binary. CPM. 6.4 - 6.48V. AB probably optical. B, 8.0v B9; C, 9.8v at 54"; D, by Wallenquist, mag. diff 7.1 at 90". AB 5.94 F3V, 7.28 F9V, 54.62y, a = 0.507". Component C, 8v at 54", optical. ADS 3605A. A* 2.98 var. A8Iap. Five visual and one astrometric components. AB visual binary, B, 14v at 29"; C, 11.26V, +1.83(B-V), +1.31(U-B), at 43"; D, 12.0v at 46". ADS 3605A, EA 2.94 - 3.83V, 9892d. Spectrum var. even outside eclipse. RV and light fluctuations about 110d. Al AnzFixed with HR 1610. Fixed with HR 1609. Colors for combined light. RRc 4.77 - 4.80V, 0.273d. S EriEA 3.70 - 3.97V, 972.164d, i 90d. Variable duration of min. Amp. depends on wavelength, 0.55B, 1.97U. K component amp. 0.05V. HaediBC binary 7.7, 10.7v sep. 0.5"; AxBC binary, B = GC 6148 A1IV?, vsini 53:k/s; D, 9.5 at 130". Probable double, 5.4, 5.4v, sep. 0.4". Optical pair with HR 1623. Gamma Cas, amp. 0.07V, period a few hours? BV CamOptical pair with HR 1622; C, 10.8v at 173" from B; D, 13.3 at 16" from B. RS CVn amp. 0.14V, 82.8d. BM CamHR mag. 6.31 should have been 7.31. A,B,C, CPM; D, optical; E, 12.3v at 132" from A. Alpha CV, 4.65 - 4.69V, amp. 0.03y, 4.6398d. V1032 OriBeta C? Hoedus IIAlpha CV, amp. 0.10U, 0.06B, 0.05V, 0.7325d. BN CamSRb 8.2 - 12.4p, 212d. Mean mag. varies in period 2450d. W OriADS 3738B, amp. 1.8v? Delta Sct 6.28 - 6.39V, 0.1352227d. X Cae5.6 G4V, 5.6 G4V, 1.19y, a = 0.18"; or 2.38y, a = 0.10"; or 5.8y, a = 0.11". Combined mag., colors. Sep. 0.099". Unresolved by speckle interferometry 1983.93. E? 5.1 - 5.6v. About 2d. A is SB, 5.7, 7.7v sep. 0.0004". Visual companions 12.0 at 13", 8.6 at 35". Primary of visual pair is possible occultation double, 6.8, 6.8v, sep. 0.3"; secondary, 9.1v at 111.5" is BD +21d764. 6.73 - 6.82p. 5.78 Am, 6.62 Am, 198.9y, a = 1.04". Mean mass 1.7 solar. Combined mag., colors. CPM with ADS 3712 = GC6270, 9.8, 8 K2 sep. 3" at 348". CursaAB, CPM. BC 8.6 dG7, 9.1, 32.1y, a = 0.217". CPM with component A. ADS 3722B, K0III-IV, RV +72k/s. 2.87d not confirmed. Suspected visual double probably single: unresolved by speckle interferometry. Candidate for becoming a Be star. Beta C 4.22 - 4.34V, 0.701538d. Both spectroscopic and new photometric data suggest period 0.70177d. Small changes in mean brightness (<0.1mag). B, dF5, optical. C observed only once. Binary. Amp. 0.003V, 0.565d. V1085 OriSRb 5.0 - 7.4v, 60:d. RX LepSRb, amp. 0.12:V, 40d. WZ DorCPM companion G8Ve, strong lithium. AB fixed. B, 8.4v, F7V at 7"; C, 11.8 at 182". AB 6.9 A4V, 7.1 A6V, 312y, a = 0.383". Combined mag., colors. C, 13v at 7", may be physical. Alpha CV 2.97 - 3.41V, per. about 2d. CPM. Combined mag., colors. Companion B9V, optical? AC binary. B, 11v F4V at 13" optical. Delta Sct 4.94 - 5.10V, 0.088088d. Form of light curve varies. Also nonradial pulsations of 0.096533 and 0.088243d. KW AurCapella is a bright binary star system whose two stars, only 70 million miles (116 million km) apart, are too close together to be seen as individual points of light with a small telescope. This star system is approximately 45 [G/light year]s distant. AP 0.6 G5III, 1.1 G0III, sep. 0.04", 0.285y, a = 0.054", masses 2.67 and 2.55 solar. Combined mag., colors. Capella is first star for which an orbit was determined from interferometer measures, by Anderson at Mt. Wilson in 1920. Speckle sep. 0.040" 1981.24 and 1981.68; 0.055" 1982.16. CPM with component H, a close binary, 10.0 dM1, 13.7 dM5 sep. 2" at 723" from A, probably physical with A. Other components all faint and distant from A. Amp. 0.03V. Variable helium and X-ray emission. CAPELLAComponent B doubtful, possibly the nebula. C 10.7V at 30". ADS 3843A, Ina 5.78 - 6.08V. Possibly a SN 2.5 million yrs. ago. AE AurThe bright blue giant star, Rigel, represents one of [X/Orion]'s feet. It is an extremely hot star, with a surface temperature over 7,000 degrees hotter than that of our [G/Sun]. As a result, it is over 57,000 times more [G/luminous] than our star. AxBC, CPM. BC binary, 7.6 B8II, 7.6v sep. 0.12". D, 15.4v at 44". BC also classified B5V+B5V. For B, vsini =<39k/s. 0.03 - 0.30V, 25d. Amp. at 0.58 micrometers about 0.06m. RIGELLb?, amp. 0.10V. PU AurCPM. ADS 3872A, E? Possible CPM with HR 1732. EA 6.15 - 6.82V, 6.05 - 6.72B, A0 + A0, 4.134695d, changing period. AR AurB, 13.4v at 29". C, 12.1v at 42" and D, optical. Possible CPM with HR 1728. Alpha CV 5.35 - 5.41V, 2.4660d. Spectrum var. same period. IQ AurFixed. Companion spectral class A. CPM. Companion 9.64V, +0.76(B-V), +0.19(U-B), G1IV-V. Component B optical. Fixed with HR 1754. Fixed with HR 1753. Alpha CV, amp. 0.04V, 2.28704d. Magnetic star. TX LepCPM. Component B optical. Fixed. Secondary 7.17V, -0.12(B-V), -0.63(U-B), B5Vn, B8nnp or B3V, RV -58k/s, vsini 350k/s, optical. AB binary; C, 9.2v K0 at 61" optical. Amp. 0.13:V. AB fixed. Companion A5IV, vsini 124k/s. CPM. Companion F6V. Companion optical. BC 7.8 F8V, 7.9 F8V, 48.0y, a = 0.34". AxBC physical. ADS 4002A is SB triple system, abc with periods 9.2y and 7.989d. Speckle interferometry gives 9.219y, a = 0.036" for for ab x c. Visual components AB, binary, 3.8, 4.8v, sep. 1.650"; C, 9.4v at 115". The total mass of the quintuple system exceeds 50 solar masses, the most massive component being about 17 solar masses. EA + Beta C 3.31 - 3.60V, 3.14 - 3.35B, 7.989268d. Also sinusoidal pulsation period, amp. 0.05V, 0.30197 or 0.30145d. Gamma Cas?, 4.92 - 4.96V, 14.50d? Amp. 0.07R, 0.06(R-I). BELLATRIXALNATHLb? 5.71 - 6.05V. SW Col359.1y, e 0.19, a 0.28", i 50.9d, mag. diff 0.3. ADS 4038A is occultation double. B and C are 10.1v at 305" and 11.8v at 343". ADS 4048A is occultation double, equal magnitudes, discovered during occultation of Feb. 26, 1901 by Innes. The three visual companions: B, 12.39V at 38"; C, 11.55V at 59"; and D, 11.6 at 74" may all be CPM with A; however, B and C may possibly be optical. AB about 6300y. B, 10.3V, vsini 96k/s. C, 12.3v at 83", optical. Ell 4.55 - 4.61V, 4.31 - 4.34B, 2.52596d. Companion F5. AB, 6.9, 7.2v sep. 0.2" binary. C, 6.8v A0. Combined mag. and colors of AB. AB binary, B is A0V; colors for combined light. C, 11.5v at 141". Companion 7.62V, +0.94(B-V), +0.69(U-B), G8III. AB binary; C, 12.0v at 64"; D, 10.5 at 206"; E, 10.5 at 241". ADS 4066B, 7.0 - 11.0v. NIHALCPM. Companion 9.70V, +0.71(B-V), +0.15(U-B), F7V. ADS 4097, cst? 4.67: -4.71V. CI OriSR? 5.9 - 7.1v, 120?d. CK Ori4.49 B5IV, 5.82 B7V, 586y, a = 1.293". Combined mag. and colors. AB fixed. Combined mag., colors. SRc 6.1 - 6.5p, 165d. CE TauCompanion is B7IV, vsini 291k/s, optical. Binary with C = HR 1851. Component B, 14.0v at 33". ADS 4134A, EA 2.14 - 2.26V, 1.94 - 2.13B, 5.732476d. Intrinsic variability also possible. MINTAKAThabitCPM. Gamma Cas, 5.53 - 5.69V. V960 TauCPM. Amp. 0.10y. All components CPM? CD binary, 8.9v A0V, 9.7v sep. 0.8" at 30" from A, physical. ARNEBEA 5.31 - 5.66V, 5.14 - 5.51p, B1V + B7V, 1.4853784d, i 80.9d. A third component has orbital period 119.09d. VV OriSuspected visual double probably single. Unresolved by speckle interferometry. Companion has K-type spectrum. See HR 1879. CPM. Fixed with HR 1887. Fixed with HR 1886. E:+SX Ari 6.54 - 6.58V, 0.94629d superimposed on SX Ari type, 0.9015d. V1046 OriBinary. COPERNICUS spectra and IR photometry yielded no evidence on the companion. ADS 4186AC fixed at 13". C = HR 1895. ADS 4186 and 4188 together appear to form one complex multiple system whose brightest components are ADS 4186C = HR 1895 and ADS 4188A = HR 1897. These two components are double star STF 17 which IDS lists as part of ADS 4188. Thus, the 9 components of ADS 4186 and the 4 of ADS 4188 form one system of at least 12 components. Those of ADS 4186 range from mag. 5.4 to 16.7v, all within 22" of A. ADS 4188 has two other companions in addition to HR 1895: B, 6.5v at 53" and C, 7.6v at 129" from HR 1897. ADS 4186A, EA, 6.72 - 6.75V, 65.43233d. Component E is NSV 2291, amp. 0.41V; component F is NSV 2296, 11.0V; component H is NSV 2292, 15.6V. See HR 1893. Fixed with HR 1896 at 13". No clear evidence for being X-ray source. Temp. 32000d excites nebulosity to 10600d. 5.10 - 5.16V. He II 4686 suggests var. density of infalling material on time scale of days. See HR 1893, 1895. 6.65 - 6.72V. ADS 4188AB fixed at 52". B is 6.38V, -0.05(B-V), -0.93(U-B), B0.5V; vsini 17k/s. See HR 1893. May be X-ray source 3U0527-05. 5.05 - 5.19V. Component B is NSV 2326, 6.38 - 6.44V. CPM. AB fixed. B is B7IV; vsini 50k/s. Component B is NSV 2334, 7.4V. Nair al SaifAB binary, both components B8IV. Combined magnitude and colors. Alpha Cyg 1.64 - 1.74V. ALNILAMGamma Cas 2.90 - 3.03V. Var. shell Sp. Widths H-lines vary in about 10 min. Polarization at H beta changes in tens of minutes, probably due to circumstellar matter. CPM. Combined mag., colors. BC, 10.0, 12.2v, sep. 11.3" at 55" from A, optical. AB 6.0 G5III, 6.3 A2V, 53.2y, a = 0.135". Combined, mag., colors. C, 8.57V, +0.28(B-V), +0.09(U-B), F0V at 12", physical; D, 11.5v at 33". Resolved by speckle interferometry 1983.93, sep. 0.12". Suspected occultation double. CDelta 3.46 - 4.08V, 9.84200d. Period varies. Component B, 9.9v M1 at 99", is BD +53d935, CPM. Component D is F5. Other companions 12.4 and 12.8v. TX PicTriple system: SB and third component 8.5v at 0.32". AB 4.1 O9.5V, 5.1 B0.5V, 170y, a = 0.247". Combined mag. and colors. C, 8.79V, A2V at 11" may be physical; D, 6.62V, -0.20(B-V), B2V, at 13" and E = HR 1932, at 42" CPM with A. A multiple system similar to trapezium. ADS 4241 possibly the most massive visual binary known, 35 solar masses. Gamma Cas 4.40 - 4.59V. Var. hydrogen emission. Lc 6.13 - 6.30V. NO AurExcept B all companions at distances 41" to 129" from A, and 5 of them mag. 8 to 10v. CPM, B is 7.18V, -0.04(B-V), -0.14(U-B), B9.5V, vsini 120k/s. 5.3 B3IV, 5.9 B3V, 95.36y, a = 0.357". Equal components. Combined mag., colors. ADS 4265B, Beta C? 6.2 - 7.0v. See HR 1948. In line of sight of high-velocity interstellar cloud. E?, 4.91 - 4.95V. Gamma Cas?, 2.62 - 2.66V. H alpha variable. Rapid variations in H beta profile. PhaetAlpha CV, amp. 0.03V, 0.04U, 1.099d. V1051 OriCPM. Amp. about 0.04V. V731 TauLb?, amp. 0.15V, 0.08R. WX MenAB 6.5 F5V, 6.9 F6V, 20.10y, a = 0.201". V1197 OriSRa 10.1 - 12.2p, 240.9d. Mean mag. varies in period 1750d. Y TauBC, 9.5, 13.0v, sep. 1.3" at 17" from A, optical. CPM with HR 1982. Delta Sct? CPM. Companion 8.97V, +0.55(B-V), +0.08(U-B), G0IV. Optical. Ell 6.00 - 6.05V, 5.288d. Additional irregular variability. Third component mag. diff 6.29V, 80" from A. Component B optical. Speculation that star may have been a SN 2.5 million yrs. ago. AB binary. C, 7.2v A0 at 75", CPM. Binary. Companion F0. EA 6.02 - 6.43V, 6.1 - 6.5p. 3.4057d. Redder at min. V1031 OriSAIPHAmp. 0.1V. Cycles 35-36d in 1970-1 not confirmed in other seasons. Companion optical. Third component, visual, 11.6v at 15". Reality of the occultation binary, sep. 0.01", has been questioned. High space velocity. Amp. 0.10V. CPM. Combined mag., color. Amp. 0.082. EB 5.12 - 5.29V, 2.933241d. TU CamHigh space velocity. Amp. 0.05U, 2.63?d. Possible new periods of 2.654 and 1.5889d, of which the smaller preferred. V809 TauWeznPossibly triple system. Magnitudes of separate components unknown. A*, 14.25y, a = 0.095". Probably low-mass companion. Optical. Beta C?, amp. <0.02V. AB optical. C, 12v at 45". Ell? 4.85 - 4.92V, 0.03b, 0.640d. EA 6.19 - 6.87V, 8.56898d. Sp. at min., B9V. TZ MenThis huge star, possibly the largest known today, is a irregularly pulsating red supergiant. Its size changes from 550 to 920 times the diameter of our [G/Sun] over the course of 5 1/2 years. At its largest, this star would completely fill our inner solar system and its surface would be extremely close to Jupiter! Betelguese is 650 [G/light year]s distant. Components B-E all 11 to 14.5v at sep. 40" to 174" from A. D 13.5 at 77", optical. Speckle interferometric observations in 1983 November (Karovska et al. 1986, ApJ, 308, 360) show A to be a triple system with closer companion at 0.06" (mag. diff. 3.4 at H alpha) and more distant companion at 0.51" (mag. diff. 4.6 at H alpha). Radio star. Circumstellar shell of gas and dust. The gas shell detached from photosphere at about 5 stellar radii. Diam of optically thin dust shell possibly 1".5. Surrounded by reflection nebula. Gas shell up to 100 R, dust shell from 12 to 250 R. Highly limb darkened. ADS 4506A, SRc 0.40 - 1.3V, 2335d. Also superimposed waves 200-400d. BETELGEUSEAll companions optical. AB binary. C, 14.1v at 13". ADS 4556A, EA 1.89 - 1.98V, 1.93 - 2.02B, A2+A2, 3.9600421d, i 78.5d. MenkalinanRadio star. Lc 4.24 - 4.34V. Radio emission at 2.85cm indicates mass loss. AB binary , combined mag., colors. B is 7.2v G2V. C, 11v at 49" optical. ADS 4566B. Alpha CV 2.62 - 2.70V. Amp. 0.43m at 1400A, 1.3735d. Magnetic field varies 3.618d. AB probably binary. B, 11v at 2". Component C, K0III, optical. 126.0y, e 0.56, a 0.265", i 75.4d, mag. diff 1.4. Delta Sct 5.88 - 5.92V, 0.0611d. V1004 OriDelta Sct 5.93 - 6.36V, amp. 0.38 B, 0.13372, 0.13612 and 0.08261d; amp. var. in 7.7455d. Multiple periods. V474 MonOptical. C, 13.0v at 20" from B. Amp. 0.15p, may be spurious due to companion. Suspected occultation double. BC, 9.0, 10.0v, sep. 0.6", CPM with A. Delta Sct? AB 4.4 A2V, 6.0 F3V, 17.5d, a = 0.276"; ABxP, 18.25y, a = 0.089". Magnitude and colors for combined light. A is alpha CVn var., SB1, 4.45d; B is SB2, 4.78d. Component C, 14v at 18" probably optical. ADS 4617A, Alpha CV 4.10 - 4.18V. Binary. Triple system, SB, sep. 0.0014". Third component found by occulation, 6.5v at 0.060". AB 4.7 G6III, 5.1 G8III, 13.17y, a = 0.19". Combined mag., colors. Component A is SB, 4.9, 6.9v, sep. 0.0013". Speckle interferometric sep. 0.128" 1982.17, 0.086" 1983.93. Component C, 13.0v at 101". PropusOccultation binary, sep. 0.02". H alpha profile var. Confusion as to whether B or C is the brighter, B at 18", C at 84" from A. C is 15v at 21". 5.20 - 5.23V, 80.85d, periodic shell phenomena. Suspected of 0.01m variability. CPM. Companion 10.72V, +0.90(B-V), +0.25(U-B), F7V. Z And 4.82 - 5.06V. H-line var. M-type component irreg. amp. 0.07y. Shell Sp. varies like R CrB. SS LepSep. 0.097". Runaway star from Sco OB1 from which it appears to have been ejected 14 million yrs ago at velocity 150 km/sec. Lb? 6.39 - 6.51V. SW PicSRb 6.0 - 7.58v, 7.1 - 8.9p, 89d, superimposed on oscillations of 875 to 890d. Amp. 0.55V, 0.08(B-V), 0.16(U-B). S LepCPM with HR 2158. Binary 5.9, 9.4v sep. 5", CPM with HR 2157. 7.2 G5, 7.4, 463.5y, a = 2.94". Amp. 0.10V. Component A is itself double, showing variable radial velocity 12.10 to 33.22k/s, and vsini 7.99k/s. One of the three components may be a spotted star. Amp. 0.13V. AB binary, combined mag., colors. C 14.4v at 18". ADS 4751B, 7.0 - 10.0v. AB CPM. B is 6.94V, +0.04(B-V), -0.02(U-B), A0V, vsini 120k/s. Component C, 8.9v at 118". HD erroneously assigned the preceding number, HD 42092, to the fainter following component of ADS 4749. Consequently the data for the two primary components are sometimes interchanged. vsini for component A is 250k/s. ADS 4749A, spectrum variable. Sometimes shows shell features. Binary with HR 2175. Old disk population runaway star. Sep. 0.099". 6.4 F5V, 6.5 F5V, 18.2y, a = 0.203". IUE observations of uv continuum suggest an early-type companion, B9 or A1III-IV. SRc 8.7 - 9.5p, 182d. TV GemAlpha CV, amp. 0.04U, 1.36:d. V653 MonLc? 5.74 - 8.1V, possibly E, per. 32y. BU GemAlpha CV 6.16 - 6.18V, amp. 0.02y, 0.724d. V638 MonEB 4.65 - 4.90V, 1.672541d. Binary. Occultation indicates sep. 0.27". Lb? 4.93 - 5.04V. UW LynAB, 473.7y, a = 1.08". B is 8.8v at 1.4". A is suspected occultation double, 3.4, 5.4v, sep. 0.03". Masses A, 12.4; B, 5.5 solar. The three components are surrounded by a gaseous envelope. ADS 4841A, SRa + EA 3.15 - 3.9v, 232.9d. Deepest min. satisfy SB period 2984d. PropusAB CPM. B is dF0; C 12.3v at 202" optical. D, 11.5v at 120" from A. B and C optical. Aitken and Wallenquist disagree on magnitude difference: Aitken AB 6.0, AC 5.3, AD 4.8; Wallenquist 5.6, 7.6, 7.3, respectively. Separation 25", 76" and 86", respectively. Companion, RV -2k/s, optical. Old disk population runaway star. Suspected occultation double, 6.9, 6.9, sep. 0.1". 6.8 F5, 7.0, 28.1y, a = 0.165". 132.7y, e 0.52, a 0.24", i 55.7d, mag. diff 0.3. E: + Delta Sct: 4.43 - 4.73V. Line widths vary 0.3d. UZ LynAP 6.1 A2IV, 9.0y, a = 0.109". B and C both 8.4v at 63" and 117", both optical. D, 11v at 5" from C. AP resolved by speckle interferometry 1983.93, sep. 0.06". Aa resolved by speckle interferometry 1983.93, but unresolved 1983.94. AB binary. B, 13.0v at 2". C, optical? 13.28V, +0.56(B-V), +0.34(U-B). Optical. 5.4 - 5.47B. AB binary. C, 12.9v at 26". D, 11.0 at 100". AE magnitude difference 6.24V, sep. 70". Amp. 0.04U, 1.0785d. H and K lines vary. V1155 OriAmp. 0.03V. AB optical. B is F8. 6.8 A3V, 7.4 A6V, 120y, a = 0.448". ADS 4971, 6.3 - 6.37V, combined mag. Difference between components varies from 0.2 to 1.5V. Uncertain which component is var. Beta C? FurudAB CPM. C at 56", optical? Gamma Cas 5.46 - 5.64V. FR CMaCPM. Lb 2.76 - 3.02V. Tejat Posterior5.48 - 5.54V. Not var. in U. Lc? 4.75 - 5.70V, 6.6 - 7.2p. Possibly faint visual companion at 50". EA 5.64 - 6.03V, 9.945070d, i 87.8d. Close third body or circumstellar matter needed to account for the light curve, but no spectroscopic evidence available. RR LynB, 10v at 31" optical; C, G8III probably optical. D, 12v at 80". Beta C 1.93 - 2.00V. Prototype star. Multi-periodic: 0.25002246, 0.2513003, 49.17 and 0.23904d, others reported. Beat periods 49.198, 5.442 and 4.900d. Sp. also var. over 0.25d. MurzimBinary with HR 2299. Combined light 4.30V, +0.21(B-V). Component C, 12.2v at 93". See HR 2298. Speckle interferometric double, 6.5, 6.9v, sep. 0.055". ADS 5023B, 7.5 - 9.0v. Lb 8.5 - 9.7p. BL OriCPM companion F0V; however, the companion is optical. IUE observations suggest an early-type companion, about A0. CDelta 5.58 - 6.62V, 27.0205d since 1933. Period has increased from 27.0093 before 1900, with mean value 27.024649d. T MonCanopus is the second brightest star in the sky. It is 116 [G/light year]s away, 30 times the diameter of our [G/Sun] and 1,400 times more [G/luminous]. CANOPUSFixed sep. CDelta 5.02 - 5.82V. Per. changing, 3.728365 before 1950, 3.728115 since. CaII emission on rising branch of light curve. Blue companion suspected. RT AurSep. 0.003". AA' probably combined light and color. This may be the SB pair, 4.3, 6.0v, sep. 0.2". B, 8.5V A1V at 113", vsini 141k/s, is binary with C, 8.9v, sep. 0.2". Component P, 15.1V at 24" optical. Other components faint at 54" to 92". See HR 2356. Amp. 0.055b. AB binary. B is K0V. Component C, 11.4v at 45" optical. Double emission lines of which red component variable intensity. Component B, 9.09V, -0.05(B-V), -0.30(U-B), B9IVe, RV +6k/s, vsini 201k/s. EA 5.79 - 6.54V, 2.52501922d. Per. changes. Rot. line apsides per. about 40,000d. WW AurCompanion F5V, optical. Optical. Quadruple system, AB 6.1 G5, 6.2, 52.9y, a = 0.484". CoD = -50d2440, 9.7, 9.8v sep. 0.5" at 12" from AB, 105.6y, a = 0.535". AB, CD are CPM. R-I also found at -0.02. Beta C 4.33 - 4.36V, 0.2095755d, secondary variations. Effective temperature varies by 1400K and ratio of max. to min. radius by 1.042. Lb? 6.28 - 6.41V. SX ColCompanion 8.70V, -0.08(B-V), -0.40(U-B), A0V, optical? Beta C, 5.64 - 5.72V. Fixed sep. SRb 7.83 - 10.00B, 8.2 - 10.0p, 234d. Mean mag. varies in per. about 3500d. UU AurH alpha emission var. A* 1.93 A0IV, 12.9y, a = 0.038". ALHENAProbably star of largest known mass for primary and secondary components, each about 50 solar masses. 6.04 - 6.08V, irregular variations, possibly transition from O- to WR-type spectrum. Polarization variable. Plaskett's starCPM. Companion 7.65V, +0.32(B-V), +0.02(U-B), F2V. AB binary. C, 11.5v at 21". Discovered by both occultation and speckle interferometry 1978, sep. 0.075"; 1983.93, sep. 0.13". 6.9 G0V, 7.3 G1V, 29.0y, a = 0.295". Combined mag., color. Companion A2V. Beta C? 6.2 - 6.25V, 7.5 hrs., possibly longest period Beta C type. Beta C?, 3.16 - 3.20V. AB binary, 4.8 Oe5, 7.6 B7; C, 9.9v B8V at 17", physical, vsini 141k/s; D, 9.7v A6III at 41", physical, vsini 115k/s; E1 the brighter component of E, B5V at 74", probably optical, vsini 253k/s; E2, A0V, vsini 132k/s. ADS 5322A, Ia? 4.62 - 4.67V. R-I also found at -0.11. S MonBinary. Companion A0. 5.58 - 5.62p. Some spectral lines appear double, indicating separation of about 110k/s and vsini of 90 and 75k/s. CPM. AB 5.37 A2n, 5.95 A2V, 699.0y, a = 1.660"; vsini of B 100k/s. C, 7.1v at 8", physical. Companion 9.22V, +1.13(B-V), +0.91(U-B), K0III-IV. MebsutaCompanion has A-type spectrum. Optical. CPM. Companion orange, optical. Delta Sct? AlzirrSee HR 2485. Color for combined light. Mag. for blended images 5.52V. Sirius, the brightest star in our night sky, is also one of the closest stars to us at only 8.7 [G/light year]s. It is 23 times more [G/luminous] than our [G/Sun] and almost twice its diameter. It has a small companion star that is believed to be a white dwarf. The companion is difficult to see because of its closeness to Sirius. AB -1.46 A1V, 8.49 A1V, 50.090y, a = 7.500" or 49.94y, a = 7.62". D, 14.0v at 32" from A. C, companion to B at 1.4" suspected but not confirmed. B is first white dwarf ever discovered; predicted by Bessel (1844) on basis of orbital motion of Sirius, it was first seen by Alvan Clark in 1862, and its peculiar high temperature, small size and great density established by W. Adams in 1925. Soft X-rays observed from Astronomical Netherlands Satellite (ANS). Sirius B not unusual compared with other dA white dwarfs. Effective temperature about 32000K. SIRIUSGamma Cas 5.13 - 5.44V. Also classified beta C, 5.10 - 5.26V. FT CMa6.81 A1V, 7.01 A2V, 1057.8y, a = 1.536". Combined mag., colors. Beta C, 5.48 - 5.76V. HP CMaAmp. 0.06V. Alpha CV 6.06 - 6.09V, 2.181d. HK CMaGamma Cas 6.15 - 6.27V. A 2-year (1977-78) minimum attributed to a dust cloud. V339 PupSRc 6.6 - 7.3p, about 47d. IS GemComponent B, 13.31V at 27.5", optical. SX Ari, amp. 0.10V. OV GemAB 5.7 G4III comp., 6.9 A2, 480y, a = 0.736". Combined mag. and color. C and D 6.3 and 6.2 pv fainter than AB. 7.1 - 7.28B. AB binary. Optical. CPM. Alpha CV 6.16 - 6.32V, 2.9760d. Magnetic field and rotation same period. Strontium var. V592 Mon7.01 - 7.06?V. Radial velocity possibly variable from +22 to +44k/s. Gamma Cas 3.78 - 3.97V, 3.7 - 3.85B. AB fixed. Space motion almost identical to that of the Sun. Delta Sct 5.94 - 6.14V, primary period 0.115442, secondary 0.154412d. OX AurAB binary. B discordantly classified B9V: or A6:, vsini 158k/s. H alpha variable. 6.52 - 6.57V. From orbit based on IUE data, the star should be eclipsing with period 195.24d. V415 CarDelta Sct 6.037 - 6.054y. About 4 hrs. One of most luminous Delta Sct stars: abs. mag. about 0.0V. V352 AurAB binary. C, 13v at 29" optical. D, 9.5 at 207". AB 4.8 A9Vp, 7.6 G6V, 1943.8y, a = 8.194". Combined mag., colors. ADS 5548A, Lb, amp. 0.22V. Emission var. about 16 yrs. Beta C 4.60 - 4.63B, 0.184557 and 0.19296d, beat per. about 2d. EY CMaLc 3.78 - 3.99V. E? 6.71 - 6.95V, 3.763d, possibly irregular. HeII 4686 var. about 13d; profiles var. in minutes. Suspected SN remnant. Companion is probably a neutron star. EZ CMaComponent B is 9.3v K5 at 44"; D, 9.5 at 130". CPM. Lb 6.25 - 6.37V. NP PupAB fixed. Old disk population runaway star. Beta C 4.36 - 4.40v, 0.08:d. Beta C 6.50 - 6.66V, 0.19d. HH CMa7.1, 7.1v, sep. 0.040". Resolved by speckle interferometry 1983.93, sep. 0.06"; unresolved 1984.93 and 1985.25. SR 5.00 - 5.07V, 6.54 - 6.64p. OV Cep6.9 F8IV-V, 7.1 F8IV-V, 16.74y, a = 0.218". Combined mag., colors. Fixed sep. ADARAAC, mag. diff 6.1v, sep. 32"; AD, mag. diff 6.1v, sep. 60"; AE, mag. diff 6.4v, sep. 50". Component B, M5III; component C, F6V, optical. Component X, K-type spectrum, optical. Gamma Cas 6.48 - 6.60V. Time scale 7d. FU CMaCep?, amp. 0.086V, 0.7282d. Sep. 0.020". Lb? 5.89 - 6.04V. NP GemOld disk population runaway star. AB binary. Lc 3.43 - 3.49V. Beta C 4.96 - 5.01V, 0.19120d, secondary 0.19740d, beat period 6.09d. V637 MonComponent A is suspected occultation double, 4.5, 4.5v, sep. 0.1". B, 10.5v at 87". C, +20d1686, 7.55V, +0.62(B-V), +0. +0.07(U-B), G1V at 96" has high proper motion, 0.100", optical, vsini =<54k/s. Other components fainter. ADS 5742A, CDelta 3.62 - 4.18V, 10.15073d. Period decreasing 3.1s/y. MekbudaAmp. 0.08V. H alpha profile changes in 30 min. or less. MuliphenAmp. 0.53:V. 5.16 - 5.32V. CPM with HR 2668 and third component, 9.2v K2 at 200". See HR 2667. Component B, 10.3v, F5III. ADS 5782A, Beta C 6.42 - 6.53V, 0.267d? or 0.18d. Other indications from 4 to 10.4 hrs. V569 MonAB binary A9V, F6V. CPM with C, 10.0v at 37". Component C, 9v at 18" probably optical. Beta C 5.36 - 5.39V, 0.12377d? FN CMaAmp. 0.026y, 3.275d. V386 CarAB optical. This star and HR 938 form a pair with opposite motion. See HR 938. Amp. 0.04b? Gamma Cas 5.64 - 5.92V. FV CMaAmp. 0.02V, 0.04U. Var. H alpha emission. WezenPossibly the center of SN explosion 0.8 million years ago. AB CPM. 4.3 - 4.36V. Component B, 11.3v, F3V. Beta C? Lb? 5.47 - 5.55V. V-R varies by 0.08m. UY LynAmp. 0.04b? Delta Sct 5.43 - 5.50V, 0.0999081 and 0.07500d, var. amp., beat per. 0.30083d. Sp. var. V571 MonAB 7.18 F8V, 7.23 F8V, 116.50y, a = 0.929". Combined mag., colors. C, 12.5v at 16" optical. Delta Sct? Difference between components B-A varies. SRb 6.63 - 7.01B, about 50d. BQ GemAmp. 0.037V, 2.68d or double. May be SB with double period. Delta Sct type. HN CMaOptical. The fainter component of the double is the variable suspect, 7.5v. Magnetic field var. 36.5d. Companion 9.07V, +0.77(B-V), +0.35(U-B), G1III or G5III, RV -3k/s, optical? Beta C, amp. 0.04V, 0.112d (variability questioned). GY CMaBinary with HR 2736. Combined light with HR 2736 varies, but 2736 is probably the variable. Binary with HR 2735. Combined mag. and colors, 3.63V, +0.91(B-V), +0.60(U-B), +0.48(R-I). 3.56 - 3.62V, blend with 2735. Amp. about 0.07u, 0.04v, 0.02b, 0.04y; 0.936d. QW PupBeta C 6.56 - 6.61V. GG CMaSR 4.80 - 4.96V, 6.40 - 6.70p, 23.7d. VZ Cam31?y. Sep. 0.098". Gamma Cas 4.42 - 4.82V. EW CMaAmp. about 0.04u, 0.01v,b,y. Combining their data with previous observations, Heck et al. (1987, A&AS, 70, 33) derive 0.91889d. OU PupAmp. 0.05V. Primary of vis. double, SRb 2.6 - 6.2v, 140.42d. L2 PupGamma Cas 3.60 - 4.18V, cycles 20 - 22 hrs. Also amp. 0.06V on time scale of 5d reported. Hydrogen emission varies with period 1.3667d (possibly a rotation period). Amp. 0.04y, 1.93d. PR PupCompanion optical. ADS 5961A is dubious occultation double, 4.0, 5.0v, sep. 0.045". B, 10.7v at 10" is CPM. Delta Sct? B, 6.01V, +0.49(B-V), dF0, optical. CPM. Old disk population runaway star. AB 3.55 F0IV, 8.18 K3V, 1200y, a = 6.975". Component A is SB, 3.7, 5.7v, sep. 0.2". WasatEB 4.84 - 5.33V, 4.5 - 4.8p, amp. 0.45V, 4.393407d. Sp. lines vary within about 1 hr. Variable polarization. UW CMaB, 10v at 8" fixed. D, 8.22V, -0.19(B-V), -0.93(U-B), B2V at 85". 3.90 - 3.96p. Possibly same period as SB. Binary with HR 2784. Component C, 10.9v at 74". Binary with HR 2783. Component D, 8.9v A0V at 215". Amp. 0.18V. NV PupEA 5.70 - 6.34V, 1.13593876d. Per. changes, possibly sinusoidally. i 77d. R CMaBeta C amp. 0.02V. 3-hour period not confirmed. Ell, amp. 0.045V, 1d. NW PupAB CPM. C, 12.7v at 42" optical. B optical. Old disk population runaway star. Amp. 0.035b. EA, 6.01 - 6.27V, amp. 0.14b, 24.6d. HQ CMaSuspected occultation double. Delta Sct? 5.80 - 5.84V. Binary with HR 2813. Gamma Cas 6.0 - 6.44V. Probably short period. Hydrogen emission also var. However, light variability questioned. OT GemPropusGamma Cas 5.00 - 5.50V. Emission lines vary in period of about one month or less. FW CMaCompanion is A0V, optical, vsini =<54k/s. AludraCompanion F5V, optical. Red giant of about 9 solar masses. Comp. A of double. Amp. 0.1V. See HR 2842. AB binary: B, 10.1v sep. 1"; C CPM. Gamma Cas 2.84 - 2.92V. GomeisaA is occultation triple, 5.9, 6.4v sep. 0.001" and 7.5v at 0.047". Visual companions B, 9.5v at 43" CPM; C, 10.5v at 146". Optical? CPM. B, 12.5v at 3" CPM. Gamma Cas 5.55 - 5.69V. FY CMaABC fixed. B, 8.1B; C, 8.6 B8V or B9p Hg Mn: at 20". Mag., color for combined light. AB 6.4 F4V, 7.5, 1090.9y, a = 3.684". C, 11.5v M0 at 21" orbital period around AB probably over 10000y. Component D, 12v at 42" optical? CPM. Companion G5V. CPM. Companion F8V. CPM? Suspected occultation double, 5.4, 7.0v, sep. 0.15". Resolved by speckle interferometry 1983.94, sep. 0.18". Ell amp. 0.051u, 0.03v, b, y. 0.6711d. Sp. period revolution about 1.4d. PS PupBinary with HR 2891. Combined colors. AB binary. Resolved by speckle interferometry 1983.94, sep. 0.24". Rapidly evolving shell. VV Cep type or symbiotic, 4.88 - 5.17V. Var. shell spectrum. KQ PupDelta Sct? 6.5 - 6.55V. Binary with HR 2910. Colors for combined light. Magnitude of blended images 5.09V. 5.5 - 5.60B. Also amp. 0.025 on time scale of 2d reported. OW PupAB fixed; B, 12.2v at 5". C, 9.71V, +0.03(B-V), -0.23(U-B), B9.5V, optical? Amp. at 0.58 micrometers about 0.10m. Companions optical. C is G type, strong lithium. AB, CPM. B, 13.2v at 26". Comp. A of multiple. Delta Sct?, amp. 0.01V, 1.5hr. Amp. 0.01B, 0.16121d. PT PupAmp. 0.02V. Triple system, components all about same mag. and within about 1". Occultation binary, sep. 0.03". Procyon is the 5th brightest star in the sky and also one of the closest. It is only 11.3 [G/light year]s away. It is twice the diameter of our [G/Sun] and 6 times more [G/luminous]. AB .35 F5IV-V, 10.3, 40.65y, a = 4.548". Binary nature first revealed in 1840 by variable proper motion; companion first seen in 1896. Component C, 11.7v at 122" optical. Delta Sct? A 0.09:d period originally attributed to the star beta CMi (HR 2845) may instead apply to Procyon, which had been used as a comparison star. PROCYONUnresolved by speckle interferometry. EW amp. 0.06V, 2.57895d. m PupBinary with HR 2949 at 10". C, 13.8v at 6" optical. Colors for combined light AB. Combined mag. 3.82V. MarkabCDelta 5.54 - 5.76V, 5.6952d. MY PupOptical. SR 5.52 - 5.72V. NZ GemAmp. >0.004y, 0.030u, 1.040d. V390 CarRS 4.13 - 4.29V, 19.423d. SRd? 6.56 - 6.64V, over 27d. Discovered by Gould 1879, variability questioned. Now confirmed by PEP observations, amp. 0.19U, larger in V. R PupAlpha CV 6.43 - 6.48V, 4.285d. Magnetic field same period. BC CamBinary with HR 2980. Colors for combined light. Blended mag. 6.34V. Delta Sct 6.43 - 6.50V, 0.09526d. AZ CMiPollux represents the head of the southern twin in [X/Gemini]. It is a yellowish star, approximately 35 [G/light year]s distant. It is a little over 4 times the diameter of our [G/Sun] and 35 times more [G/luminous]. All the visual companions optical. NSV 3712 is component A, 1.10 - 1.17V, while component E is NSV 3716, 10.5v. POLLUXVar. in red and IR. Amp. 0.24R, 0.20(R-I). D. W. Dunham gives 5.8, 5.8v, sep. 0.1". Amp. 0.07b? Binary with HR 3010. E, amp. 0.41y, 1.660d. Equal components. PV PupBinary with HR 3009. C optical. Some disagreement as to which of B and C is the brighter. H alpha emission var. Amp. 0.03b. Amp. 0.2V. QY PupAmp. 0.18V. Binary. Companion dG3. 2.41d, 0.06V. OX PupSR? Amp. about 0.02V. R-I also found at +0.06 and +0.07. Cst 6.14V. T PupAzmidiskeAmp. 0.5p. Binary, 211.8y, e 0.17, a 0.265", i 59.1d, mag. diff 0.2. Companion B9V, RV -72k/s, optical. Beta C, amp. 0.015u, 0.1182d. QS PupSRb 6.14 - 6.42V, about 35d. BC CMi5.6 F9V, 6.2 G4V, 23.18y, a = 0.58". Combined mag., colors. Masses 0.86 and 0.99 solar. Optical. 6.4 F2, 6.7, 30.8y, a = 0.295". BetaC, Amp. 0.03b, 0.040u with large modulation. Primary period 0.1927d with secondary 0.1680 or 0.2019d. QU PupBinary. a PuppisBeta C or Ell?, 4.47 - 4.54V, amp. 0.07y. QZ PupBeta C Amp. 0.027V, primary period 0.1160d with secondary either 0.1168 or 0.1323d. V372 CarLocated just inside 3U0750-49 error-box. HeI 4026 varies, 1.3295d. 7.0 F5V, 7.1 F7V, 57.04y, a = 0.44". Combined mag., colors. Amp. 0.42V. PX Pup6.4 - 6.58V. Occultation double. Alpha CV 5.95 - 6.08V, 8.0278d. 1.14d also possible. Length of period varies in cycles 1.8 yrs. Magnetic and spectrum variable 8.0269d; also rotation period. AX CamAmp. 0.03b? Soft X-ray source. Beta C, amp. 0.015V, 0.101d. RS CVn?, amp. 0.06V, 10.163d. AE LynL 6.2 - 7.10V. IR observations of red giant in reflection nebula suggest star is losing mass and becoming a planetary nebula. Circumstellar reflection nebula probably related to a hotter companion. V341 CarComp. A of visual double, EB 4.74 - 5.25p, 1.4544877d, contact binary, equal components. V PupGamma Cas?, 6.48 - 6.63V. Amp. at 0.58 micrometers about 0.10m. FK Com, amp. 0.020V, 0.025B, 0.030U, 0.207878d. V645 MonCPM with HR 3143. CPM with HR 3142. Amp. 0.03B pulsating. Gamma Cas 5.72 - 5.84V, period a few days. H alpha variable. V374 CarAmp. 0.04v, 6.82d. PY PupAmp. 0.07(U-B). Companion B9IIIp. Amp. 0.15V. Fixed sep. Companion 8.77V, +1.30(B-V), +0.07(U-B), M6III, optical. May be Mira-type variable. Amp. >0.022, 2.008d. V336 PupBinary. Combined light and colors. With HR 3207, appears capable of producing most of the observed ionization of Gum Neb. Change in H alpha emission profile between 1974 and 1976 interpreted as change in rate of mass loss. NaosLb 5.97 - 6.04V. Lc? 5.2 - 5.44V. MZ PupB is A0. BC double 8.6, 13.0 sep. 1". Component B, 8.66V, -0.09(B-V), -0.52(U-B), B9IV. Companion not confirmed. Delta Sct 2.68 - 2.78v, 0.14088143d. Companion K0. Beta C, amp. 0.04V, 0.264 or 0.359d? V375 Car6.70 - 6.80p. B, 10.1v G8II at 33" optical. C is K2III. Psi2 Fl 14 CncCompanion A5III, optical. Old disk population runaway star. PQ PupOld disk population runaway star. Components B6V and B9V. See HR 3206. Mag. and colors blended with other companions. C = CoD -46d3848, 7.65V, B6V at 63", physical. D, 9.07V, Am at 94", SB, over 7d?, optical. Low degree of polarization indicates symmetric shell. The brightest O-type star and one of only four WR stars bright enough to have been observed spectroscopically in UV by COPERNICUS. With 3165, appears capable of producing most of the observed ionization of Gum Neb. The brightest and presumably the nearest Wolf-Rayet binary. Radio emission interpreted as coming from circumstellar gas cloud extending farther than the orbital radius of the binary. 1.6 - 1.8V, 154 sec. Sp. var. in about 200 sec. Variability too great to be explained by the 78.5d SB companion. Possibly a third close companion: a collapsed star of less than 2 solar masses. Suhail al MuhlifCombined mag. and color for 3208-9-10, 4.67V, +0.53(B-V). AB 5.63 F7V, 6.02 F9V combined colors (AB), 59.7y, a = 0.884". Component C = HR 3210. TegmenBetaC, Amp. 0.018u, 0.108d. IS VelAlpha CV 5.53 - 5.65V, 4.116d. BM CncSuspected occultation double. Lc 4.4 - 4.5V. NS PupCep 5.50 - 5.86V, 4.22717d. Per. and form of light curve vary. AH VelB, 9.78V, +0.39(B-V), -0.02(U-B), F5IV. Gamma Cas 4.60 - 4.88V. H alpha variable. MX Pup4.60 - 4.71p. OS PupCompanion K5V, RV +7k/s, optical. Amp. 0.03b. E? Amp. 0.062. M 6.2 - 11.8v, 361.43d. R CncCPM. AltarfCPM, A2IV, F2V. Delta Sct 6.29 - 6.33V, 0.0755d. Some intervals of constant brightness. HQ HyaAlsciaukat7.1 A, 7.4, 435y, a = 0.654" or 241.4y, a = 0.569". Companion A2V, optical. AB, sep 0.100", unresolved by speckle interferometry. 7.9 - 8.03B. CPM with HR 3302. CPM with HR 3301. C, 8.5v at 38" from B, binary. E? 1.82 - 1.94V, 3.57 - 3.83p, 785:d. AviorSee HR 3310. Binary with HR 3313. B, K1III optical. SRb 5.41 - 5.75V, about 40d. BP CncDelta Sct? 5.58 - 5.61V, 54.71 min. LM HyaB is 15v at 7", CPM. C and D optical. 3.3 - 3.8V, 358d. Also 0.05d, amp. 0.02V. MuscidaBinary with HR 3328. EA 6.7 - 7.14v, 1.25686d. NO PupDelta Sct, amp. 0.025V, 2.3 hours. CX CncComponent B, CoD-51d3003, 10.2v, B8V, optical. Third component G3V may be physical. Uncertain if double or triple; 6.4, 6.9, sep. 0.25", other possible component 7.0v at 3". Occultation obs. uncertain. E amp. 0.3p, 4.56960d. Equal min. Redder at both minima. VV PyxAB 7.1 A5m, 7.2 late F, 53.0y, a = 0.321". C, 10.5v at 18" binary around AB. EA 6.37 - 6.61V, 2.49955d = SB period. Secondary eclipse amp. 0.06V; primary not yet observed. LO HyaAP 6.6, 6.6v binary. Combined mag. and colors. B, 9.7v at 25" optical. Companion 10.3v, F2V, optical? Delta Sct amp. 0.015V, 0.07:d. GU VelCPM. ADS 6872B, L 9.0 - >12v. H alpha emission var. Occultation pair 6.4, 6.4v, blended mag. and colors. Visual component 10v at 63". Suspected as double by Innes from observation of occultation of April 28, 1898 (references: Astron. Nachr. 150, 423, 1899; MNRAS, 61, 416, 1901; Cape Ann. 2, part 6, 1907). Theta Cnc B is NSV 4117, 11.5v at 58", 59d. AP, 6.4, 6.4v, sep. 0.176", combined mag., color. Components B, 7.7v at 4" binary with AP, C, 9.3v at 19". Components B2III and B2.5V. Equal components reported; however, duplicity not confirmed. Delta Sct? 5.6 - 5.67V. Lc? amp. 0.27B. AB 6.9 A7, 7.0, 136.5y, a = 0.568". Combined mag. and color. VX PyxSKYLAB indicates cool star with hot companion. Old disk population runaway star. 5.8 - 5.89B. MuscidaCPM with HR 3396. See HR 3395. 7.2 G5IV-V, 7.2 G5IV-V, 13.9y, a = 0.160". Combined mag., colors. Alpha CV 5.66 - 5.76V, 5.57d or 11.305d, double wave. Rotation, same period. Spectrum var. Magnetic field 4.606d. HV HyaComponents M1IIIa and G7IIIb. Amp. 0.09V. MuscidaAmp. 0.025y, 2.67d. Spectrum var. same period. HV VelAl Minliar al ShComponents B, 6.60V, +0.01(B-V), +0.03(U-B), A0III at 150", vsini =<40k/s; P, 9.22V, +0.39(B-V), +0.01(U-B) at 134"; and Q, 8.81V, +0.32(B-V), +0.09(U-B), F2V, at 135", vsini 86k/s, form a physical system with A. B is 40 Cnc; Q is +20d2161. ACD a physical group: C, 7.70V, +0.20(B-V), +0.16(U-B), Am, vsini <45k/s. D, 9.39V, +0.41(B-V), +0.03(U-B), F5V at 83". B, 10.37V, +0.59(B-V), +0.11(U-B), G0IV-V at 21", CPM. AB 5.3 G3V, 6.7 K0V, 145.0y, a = 1.700" or 140.0y, a = 1.8884". Combined mag., colors. Amp. 0.05v, 1.43d. 6.5 F3IV, 7.6 F6V, 66.5y, a = 0.527". Combined mag., color. Companion A2V. Amp. 0.02V, 0.26145d. Probable beat phenomena. HW VelOptical. CPM? Companion F0IV. Component A of double. Ell?, 5.17 - 5.27V. Beta C 3.56 - 3.67V, 0.131977d. Beta C?, 5.56 - 5.62V, amp. 0.01b, 0.388d. Possibly the shortest period known for a He-weak star. Component A suspected occultation double. Three visual companions. Asellus BorealisBeta C 4.27 - 4.33V, 0.17d. Beta C 4.3 - 4.33V, amp. 0.04B. V343 CarAP, suspected double, unresolved by speckle interferometry. Visual companion 12.2v at 38" optical. Asellus AustraliUnusually high-velocity interstellar CaII not associated with galactic rotation, but probably part of Vela supernova remnant associated with Pulsar 0833-45 about 3d away. Amp. 0.037b, 0.563d. HX VelAlpha CV 5.58 - 5.71V, 4.2359d. BI CncBinary with HR 3467. Component C 8.0v at 0.5" from B. Alpha CV, 5.49 - 5.56V, 3.376d. KT VelSee HR 3466. Amp. 0.015b, 0.0284d. HY VelBinary. Companion is dF3. Binary with HR 3475. The magnitude difference between HR 3474 and 3475 appears to vary. Binary with HR 3474. Probably NSV 4238. 5.6 - 5.70B. AB 3.8 G5III, 4.7 A8IV or F0V, 15.05y, a = 0.238". Speckle interferometric sep. 0.263-0.272", 1980-3. Combined mag., colors. ABxC, 3.4, 7.8, dF7 at 3" from AB, 890y, a = 4.536". Component D, 12.7v at 19" from A, in hyperbolic orbit about ABC, periastron distance, 29". AB binary with CPM double companion CD at 69". CD 11.0, 13.5v sep. 6". H alpha emission var. Components B8III and B7IV. Component B, RV +24k/s. 6.30 - 6.40V. CPM. Wide CPM pair with HR 3496. See HR 3494. Gamma Cas 4.4 - 4.50V. Variable H alpha. V344 CarAlpha CV, amp. 0.02V, about 6d. KX HyaSep. 0.05", but duplicity doubtful. Delta Sct, 0.087d. HZ VelLb? 6.23 - 6.37V. BO CncCPM. AB binary. Other components optical. ADS 7050. Uncertain which component varies. B-A discordant by over 2.0v. EA 6.02 - 6.66V, 1.6698684d. Also Delta Sct amp. 0.04V with possibly changing period, 0.074 - 0.097d. RS ChaCPM. AB binary. B is K0. SRb 5.6 - 7.5v, 9.3 - 10.9p, 195:d. X CncBinary. Combined mag., colors. Suspected occultation double. 6.1 Am, 6.1, 7.24y, a = 0.1036". Combined mag., color. Binary with HR 3552. Colors for combined light. Blended mag., 6.08V. Levato indicates spectral classes G5III+A0V, both vsini =<50k/s. IDS gives two other components. CD, both 11v sep. 2.5" but does not indicate separation from A or B. Amp. 0.04:V. Multiple periods 1.97, 1.73 and 1.66d found, but subsequently questioned. IY Vel7.0, 7.0v; combined mag., colors. Unresolved by speckle interferometry. Amp. 0.08(B-V). BC 10.8, 11.0, 39.69y, a = 0.68". BC is dM1. BCxA: 817.91y, a = 9.092". Separation rapidly decreasing. ADS 7114Aa, 11.02y, a = 90.354". This is the SB pair. ADS 7114A, S, 3.12 - 3.18V, 0.071d. TalithaADS 7115A is questioned close double. Combined mag., colors, 5.0, 5.0v, sep. 0.1". B is 10.8v at 11", binary. AcubensAB 4.11 F5V, 6.18 G5V, 21.85y, a = 0.619". Combined mag., colors. Companions C - E optical. Masses A, 1.13; B, 0.84 solar. Fixed. B is B9.5V. vsini both components 0k/s. Beta C 4.91 - 4.96V, amp. 0.015b, 0.0208d. V376 CarAB fixed. Delta Sct 5.15 - 5.17V, 0.065d. FZ VelCPM. Companion F3IV. Beta Cep 6.02 - 6.06V, about 7 hrs. with beat phenomenon. IU Vel4.2 A0IV-V, 4.4 A0V, 70.1y, a = 0.27" or 64.29y, a = 0.26". Mag., colors for combined light. Alpha CV 5.33 - 5.49V. Spectral-line intensities vary with period 4.191d. Optical. Amp. 0.03:V. Multiple periods 9.64, 14.4 and 10.7d. IZ VelAB 4.85 F7IV-V, 8.16 K2V, 1067.1y, a = 6.20". C, probably optical. ADS 7203B, 7.5 - 10.0v? AB binary. B is F5V. C, optical. Binary. Triple SB system. Combined mag., colors. Alpha CV 5.22 - 5.27V, 5.0035d. B, optical. Unresolved by speckle interferometry. Young disk population. Lc 2.14 - 2.22V. AlsuhailSRc? 6.2 - 7.7p, 120d. Mean mag. varies in period 1700d. RS CncUnresolved by speckle interferometry. Gamma Cas 4.67 - 4.78V. V345 CarBC, 10.5, 10.8v, sep. 0.3", CPM? Noted by W. Herschel as double, sep. 49", is probably error: single star. AP 7.2 G9V, 7.2 G9V, 2.65y, a = 0.126". Resolved by speckle interferometry 1983.94, sep. 0.17". Combined mag., colors. Amp. 0.07V. GX VelEA 6.11 - 6.58V, 7.750d. Misnamed KM Hya in the 64th Name List of Variable Stars (IBVS 1581) and propagated in IBVS 2015, the KM designation having previously been asigned to a faint star. HR 3655 has now been corrected to KW Hya (IBVS 2681). KW HyaE 3.41 - 3.44V, 3.20 - 3.56p, 0.05R, 6.751154d. a CarAB 6.7, 7.2v sep. 0.11". Combined mag., colors of ABC. KL VelDelta Sct? Amp. 0.03V, 3 hrs., but sometimes cst. for 5 hrs. DD UMaHelium var.? AB optical. 6.3 - 8.1p. Binary, combined mag., colors. Balmer lines show quasi periodic var. in cycles of about 35 min. Miaplacidus6.3 - 6.34p. Optical. AB binary. Amp. 0.04b. 5.08 - 5.14V. AB, mag. diff 4.6v, binary. Lb 5.87 - 5.95V. CG UMa2.2 - 2.5:v. TuraisAB 6.50 F3V, 6.74, 389.05y, a = 1.516". Binary. AB CPM. BC, 6.87v F5V, 9.0v K2V, sep. 9", physical. B, 7.04V, +0.35(B-V), +0.03(U-B), vsini =<60k/s. AB 6.1 F4V, 6.1, 3.2y, a = 0.124". CPM. Components B9V and A0V. Close to error box of X-ray source 3U0918-55. AB binary. C, 10.0v at 7", CPM? AB 7.3 A2, 7.4, 58.93y, a = 0.150". Combined mag., colors. Alpha CV 6.51 - 6.53V, 33.97d. KU HyaCPM. 5.72 - 5.76V. AB binary. NSV 4478 is ADS 7351B, 9.5 - 11.5v. Al Minliar al AsThird UHURU Catalogue suggests Kappa Vel as optical counterpart of 3U0918-55, but HR 3717 is much closer. AB combined mag., colors. C, 11.5v at 10.7". All three CPM. Alphard, the "Dragon's Heart" in the [G/constellation] of [X/Draco], has a reddish tint to it. This slightly variable star lies approximately 140 [G/light year]s away. ALPHARDCPM. CPM. 5.87 dF8, 6.53, 116.85y, a = 0.875" or 118.227y, a = 0.880". CPM. AB binary. C, 10.5v at 100", optical. Delta Sct, amp. 0.07B, about 2 hrs. CPM. Amp. 0.025V, pulsating. Optical. Amp. 0.058V, 0.9202d, pulsating. DK UMaSp. var., 7 - 12d. AlterfCPM. Companion 9.54V, +0.44(B-V), +0.03(U-B), F6V. CPM with HR 3781. Suspected occultation double. 4.1 F2IV, 4.6 F0V, 33.99y, a = 0.795". Combined mag., colors. Comp. B, 4.5 - 5.1v. Optical. Spectrum var.? EW 6.4 - 6.92V, 6.7 - 7.22B, 0.648345d, per. probably varies. S AntSuspected double unconfirmed by speckle interferometry. Amp. 0.012y, 40.4d. Possibly rotational modulation from active regions. SU LMiL? 3.10 - 3.16V. N VelBinary. Secondary F0. AB fixed? B is F5. C, at 118". Probably optical. Heis-Argelander Binary? Amp. 0.033y, 18.0d, possibly due to rotational modulation. SV LMiSecondary B8V, vsini 157k/s. CPM. Companion F8V. Discordant magnitudes and colors: Nicolet: A = 7.86V, -0.10(B-V), -0.43(U-B); B = 9.07V, +0.55(B-V), +0.01(U-B). USNO Photoelectric Catalogue: A = 6.36V, +0.01(B-V), +0.03(U-B); B = 9.51V, +0.50(B-V), +0.03(U-B). Component A suspected occultation double. Suspected occultation double; possibly SB. Amp. 0.05V, 2.8519d. Also pulsations of 11.67 min. IM VelCPM. CPM. Lb 5.84 - 5.98V. DR LeoComponent B, 9.9v at 85". Subra4.4 - 4.44B. Companion G8V, RV +14k/s, optical. R-I also found at -0.04. High velocity star. 5.06 - 5.17V, 0.04R. 6.0 A2, 6.1, 10.72y, a = 0.142". Combined mag., colors. Amp. 0.16p. CS UMa5.4 F7V, 5.6 F8V, 18.32y, a = 0.134". Combined mag., colors. E amp. 0.2b. Component A of visual double. IP VelCep amp. 0.1V, period a few days. Ras Elased AustrBinary 7.0, 7.2v, sep. 0.031", resolved by speckle interferometry at 4-meter Mayall telescope, but unresolved 1983.96 at Pic du Midi. Combined mag., colors. 6.5 - 6.59V. CDelta 3.28 - 4.18V, 35.53584d. Period varies. l CarCPM. Delta Sct 3.77 - 3.86V, 0.133d, amp. and form of light curve vary. AB, about 200y. B also A8IV. Comp. B of visual double, Delta Sct 6.08 - 6.12V, 0.08184505d. DG LeoSee HR 3890. 5.30 A3IV, 5.38 A3IV, 105.5y, a = 0.360". Combined mag., colors. Secondary B9. Ras Elased BoreaAB 5.58 A1V, 6.07 A4V, 77.55y, a = 0.383". Combined mag., colors. C, 12.28V at 36" optical. Binary. Cst? 5.23V. SY UMa6.3 - 6.36B. BetaC, Amp. 0.03b, 0.1096d. Binary. Combined mag., colors. Amp. 0.13V. Companion K0III, optical. BetaC, amp. 0.013b, 0.1608d. IV VelCPM companion A0III; however, the companion is optical. Amp. 0.24V. CPM. Amp. 0.10V. Fainter component is BD+32d1968. Probably optical. AC binary. B, 12v at 12" optical. C, 7.0v A0, vsini 50k/s. Suspected occultation double. Delta Sct? 4.47 - 4.52V, about 0.1d. Binary, sep. 0.097", unresolved by speckle interferometry 1982.17. 5.3 K0IV, 6.9 G5V, 232y, a = 0.64". Combined mag., colors. Cst 6.49V. R VelABxC, CPM. C is 13.0v at 28". CPM. Regulus, the heart of [X/Leo], is the star at the base of the "Sickle of Leo". It is approximately 75 [G/light year]s distant. It has a small companion star which lies approximately 4,660 [G/A.U.]'s from Regulus. AB binary, B, 8.13V, +0.86(B-V), +0.51(U-B), K1V. BC, 7.6, 13.1v, 2000y, a = 4.163". REGULUSVisual companions both optical. CPM. M 4.5 - 9.9v, 149.49d. S CarLb? 6.1 - 6.40v. V368 CarCst? 6.25V. U UMaSuspected hard X-ray source. Gamma Cas 5.63 - 5.83V. QY CarAB binary. Both A and B Am stars. vsini both components =<25k/s. B is 7.36V, +0.30(B-V), +0.19(U-B). 7.2 dF2, 7.5, 552.0y, a = 1.299" or 810.5y, a = 1.198". Combined mag. Primary unresolved by speckle interferometry 1982.17. AdhaferaTania BorealisCompanion is M1. 6.9 A5V, 7.0 A5V, 124.0y, a = 0.435". Combined mag., color. Amp. 0.32V, 0.11R. GY VelAlpha Cyg: 5.30 - 5.65V, amp. 0.65U, about 140d. AG AntLc? 3.36 - 3.44V. V337 CarDelta Sct?, 4.77 - 4.83V. See HR 4057. See HR 4057. 6.37 - 6.44P, 0.21R. GZ VelCst? Comparison star was the var. RS SexCPM? Combined mag., colors. Components A1V and A1Vn. E?, 2.99 - 3.33V. Tania AustralisProbably not var. Comparison star was variable. Alpha CV?, 4.91 - 4.99V. AB binary? Spectrum and H alpha vary. Amp. 0.025y, 4.37d. Spectrum var. SS SexB, 13v at 8", optical. SRb? 5.60 - 5.67V, 1 - 2d? DE LeoPossible He var. CPM. 4.40 G8III-IV, 6.12 F8V, 37.92y, a = 0.340". Combined mag., colors. Primary is occultation double, 6.7, 6.7v, sep. 0.02". Alpha CV 5.97 - 6.15V, 7.897d. Magnetic var. 7.9d? and var. Sr, Cr. CX LeoPossible small amp. variations with proposed periods of 3.57, 0.64d rather uncertain (Manfroid and Mathys 1985, A&A, Suppl. 59, 429). Amp. 0.07B, 0.06(B-V), 0.14(U-V), 58.82d. V399 CarAmp. (U-B), 0.13. Triple CPM and common RV system. B = BD+56d1458, 9.94pg; C = BD+57d1266, 8.99pg. 3.79 - 3.83V. Companion F9Ve, strong lithium. Primary is SB. Slight variation with period or half-period of about 8d suspected. AB CPM. B is F6V. C, 9.5v at 64" optical. Optical. B = CPD-60d1944 = HD 91269, 7.54V, -0.08(B-V), -0.57(U-B), B5Vne, shell star. Visual companion optical. 4.4, 4.8v, sep. 0.11"; combined mag., colors. Old disk population runaway star. Alpha Cyg 3.83 - 3.90V. Companion K5, optical. Fixed with HR 4136. Mag. and color for combined light, 5.16V, -0.15(B-V), -0.62(U-B). See HR 4135. Gamma Cas 3.27 - 3.37V. PP CarCPM? Companion spectral class A. Alpha Cyg, amp. 0.1v, 0.05y, cycles 15 - 20d? Irregular var. in H alpha emission profiles indicating chromospheric activity. V369 CarA is SB. Visual companion 8.5v at 2.4"; CPM. ADS 7837A, EA 5.66 - 5.75V, 2.4450566d. TX LeoAmp. 0.08(B-V). Lb 8.1 - 9.7p. Amp. 0.25V. U AntPhi16.7 F4V, 7.5 G0V, 210.1y, a = 0.982". Combined mag., color. Optical. Companion A8III, optical. SRb 7.0 - 9.2p, 7.0 - 9.4B, about 450d. Amp. 0.12V in one cycle in 1971. U Hya4.2 F3IV+F0V, 5.1 A6V, 16.30y, a = 0.340". Possible abs. mag. = -8.0V. Alpha Cyg 5.45 - 5.52V, amp. 0.035y. V370 CarPhi in most cataFixed. Combined mag., colors. Companion A5V. Optical. Probably CPM. B is B8. C, 11.2v at 20" from B. SRb 5.98 - 6.16V, 150d. RX LMiLambda 4200 star. Alpha CV 5.48 - 5.52V, 1.6731d. Magnetic field varies with same period. Relative to HR 4205, delta u = 0.102, delta y = 0.046. V364 CarOne of only four WR stars bright enough to have been observed spectroscopically in UV by COPERNICUS. Companions optical. AB CPM. B is GC 14751, dG0. AB binary. B is K0III. Lb 5.89 - 6.5v. VY UMaSpectrum var., 1.7788d. Discussion of earlier suspected period of 0.7045d given by Walborn (1979, PASP, 91, 442). vsini 202k/s. High speed mass ejection. Sep. 0.03", but duplicity doubtful. Amp. 0.028y, 0.038u, possibly eclipsing. Intervals between minima about 3d. Old disk population runaway star. CPM with HR 4212. CPM with HR 4211. 2.7 G5III, 6.4 G2V, 116.24y, a = 1.437". Secondary also classified F8:V:. Old disk population runaway star. Suspected amp. 0.08V on time scale of 2 hrs. Amp. 0.09 in (B-V). Old disk population runaway star. PraecipuaCPM. Companion 8.75V, +0.58(B-V), +0.01(U-B), G0V, RV = +18k/s. B, optical. Amp. 0.2V. Suspected visual binary unresolved by speckle interferometry. 3.76 - 3.80V. See HR 4259. Appears to be variable over long time scale, especially toward uv (may be constant in V). KQ VelAB 6.1 F2III, 8.0, 128.34y, a = 0.823", or 90y, a = 0.75. Visual primary is SB, sep. 0.001". Lb? 5.69 - 6.03V. VY LeoCst? 7.00B. T CarAmp. 0.02B, 0.150d. IW Vel6.0 - 7.4p. Faint only Feb. 6, 1943. CDelta 5.72 - 7.02V, 38.7681d since 1939. Period varies, earlier 38.753d. U CarAlkesSuspected occultation double. Optical. MERAK1.87 K0III, 4.81 F0V, 44.4y, a = 0.603". Also classified K0II-III + A8V:. Combined mag., colors. Also CPM at 280" with HD 95638 = GC 15179, 7.12V F8; SB, 6.04d. ADS 8035A; B also var. suspect NSV 5071, too close to primary to be certain of variability. DUBHEUnresolved by speckle interferometry. Suspected occultation double. CPM. AB, CPM. 5.6 F4V, 5.7 F4V, 7.40y, a = 0.140". Combined mag., colors. Blue straggler. EA 5.65 - 5.94V, 2.267701d. Chi2 Hya7.2 - 7.37B. Alpha CV, amp. 0.03V, 2.433d. V815 CenAmp. 0.02b. Large spectrum var., 0.8183d (not confirmed). Amp. 0.02V. HR 4340 used as comparison star. Lb? 5.79 - 5.95V. CO UMaDelta Cep? 3.84 - 4.02V. V382 CarAlpha Cyg 5.12 - 5.19V, amp. 0.055y, 15 - 20d cycles. Also var. H alpha profiles indicating chromospheric activity. V371 Car6.7 B9V, 7.1 A1V, 233.0y, a = 0.383". Astrometric binary. Combined mag., colors. Fixed sep. Fixed sep. Component A of double; Cep?, 4.58 - 4.62V. Companion A0, optical. Delta Sct? ZosmaChortAmp. 0.03b, 0.58:d. Lb?, 4.59 - 4.65V. CPM. If secondary is on main sequence, the spectral class is inferred to be F1V. AB CPM. B, 11.5v at 1". C, optical. ADS 8115A, brighter component of the SB system, Alpha CV 6.32 - 6.35B, 5.90513d, two unequal max. Same rotation and magnetic per., related var. EuII and SrII emission. SV CrtPrecedes HR 4369 because 1900 position given in HR, (Harvard Annals, Vol. 50), is erroneously 11.9 instead of 11.8m. AB 4.32 G0V, 4.79 G0V, 59.840y, a = 2.530". Combined colors. Mag. for blend 3.79V. AB, first visual double for which an orbit determined, in 1828 by Savary. Third component astrometric with A, 1.832y, a = 0.055". See HR 4374. Alula AustralisCPM. Alula Borealis6.0 - 6.6V. 4.3 B5VN, 5.0 B6V, 39.18y, a = 0.277". Combined mag., colors. 4.03 F2IV, 6.70 G3V, 192.0y, a = 1.92"; possible subsystem with period about 16y. Combined mag., colors. Combined mass about 3 Suns. Delta Sct? Sep. 0.0034", discovered by occultation. Companion not confirmed. AB 6.51 K0IV, 7.57 K2IV-V, >4000y. Combined mag. 6.16V. C, 9.9v at 90" probably physical. ADS 8175AB, 8.2 dG5, 4500y. Primary SB. Visual companion A3V. Ell:, amp. 0.13V, 39d x 2? EE UMaSR, 3.78 - 3.86V, about 1100d. Gianfar5500y. Circular orbit. Companion, K6IV. Alpha Cyg 6.31 - 6.36V. V809 Cen5.75 F6V, 7.07 G3V, 72.87y, a = 0.813". Combined mag., colors. Possibly wide physical pair with HR 4442. SRd 5.8 - 6.6p. At times shows cycles about 200d. See HR 4441. Alpha Cyg 5.12 - 5.22V, 46.3:d. Omi2 CenCPM with HR 4444. Binary. AB binary. Combined mag., colors. B is B6. C, 9.64V F5 at 63". SRb 5.55 - 5.80V, about 60d. V763 CenAB long period binary. C, 11.17V at 21" optical. Companion B9V, optical. Duplicity doubtful. Lb 5.23 - 5.37V. CPM. AB binary. CPM. Amp. 0.09V. 5.5 G0, 6.3 A0, combined mag., colors. GT MusAmp. 0.13V. Resolved by speckle interferometry 1986.44, sep. 0.03". AC CPM. C, 8.44V, +0.50(B-V), +0.035(U-B), F7V. SRd 4.95 -5.12V, 130:d. Spectrum var. F5-G0Ia-O + B1Iab. At blue edge of instability strip. V810 CenOptical. Amp. 0.08V. Amp. 0.04V? Discordances as 7.0 - 7.12p RS, amp. 0.03V, 71.7d. DQ LeoLb 4.6 - 4.8V. 6.0 A8V, 8.3 G2V, 122.0y, a = 0.68", 180y, a = 1.00". Combined mag., colors. ADS 8311B, 7.5 - 9.5V. SRb 4.85 - 5.12V, 61d. II HyaRepresenting [X/Leo]'s tail, Denebola lies 40 [G/light year]s away and is approximately 20 times more [G/luminous] than our [G/Sun]. B, 15.7v at 40" physical; C, 13v at 80" optical. Delta Sct?, 2.09 - 2.16V. DENEBOLACompanions optical. ZavijahSuspected occultation double. Combined mag., colors. The reality of the companion, CF UMa, announced by P. van de Kamp (see Low Luminosity Stars, ed. S. S. Kumar, p. 199, 1968) has been questioned (PASP, 96, 557, 1984). Unresolved by speckle interferometry 1980.47. Companion of Groombridge 1830, UV? 8.5-12v. Groombridge 1830Alpha CV, amp. 0.04V, 0.04B, 2.344d. PHADCPM. Combined mag., colors. Binary with HR 4561 = ADS 8347D. AB binary 7.2, 9.0 sep. 0.3". ABxC, 8.4 at 4" also binary. Amp. 0.09B, 0.87d? Uncertain which of components A, B, C of ADS 8347 is the var. DN UMaSee HR 4560. Discovered as double by W. Herschel, sep. 90" but no visual companion subsequently seen at that separation. LV HyaUsed as comparison for HR 4603; uncertain which is the variable. AB, CPM. B, 12.5v at 7". D, 12v at 140". Doubtful if double. Optical. Fixed sep. Old disk population runaway star. Delta Sct amp. 0.02V, 0.04d - 0.08d, possible beat phenomena. DP UMaBinary. Companion A9V. vsini both components =<50k/s. Beta C 4.70 - 4.74V, 0.0889d. See HR 4573. The2 CruUnresolved by speckle interferometry 1982.17. CPM. ADS 8417B, 10.4 - 11.4?v. AB combined mag., colors. C, 8.2v A3 at 9", CPM. CPM with HR 4619, 4621. H alpha varies. CPM with HR 4618, 4619. Gamma Cas 2.51 - 2.65V. Expanding circumstellar shell. AlchibaEA 5.75 - 5.94V, 4.966377d. V788 CenGamma Cas 5.47 - 5.58V, 5.4 - 5.6B. V817 CenMinkarCDelta 5.89 - 6.49V. Period changes 9.66011 to 9.66007d. S MusAmp. 0.28V. Old disk population runaway star. CPM. Binary. Combined mag., colors. Beta C 2.78 - 2.84V, 2.25 - 2.31p, 0.151038d. Expanding circumstellar shell. MEGREZ6.8 F5, 7.9. Old disk population runaway star. Expanding circumstellar shell. Gienah GhurabRS Cvn, amp. 0.19V, 63.15d. DK DraBinary. Companion 8.77V, +0.57(B-V), +0.09(U-B), F7V. Delta Sct amp. 0.04B. SRb? 3.99 - 4.31V, 40d. CPM. Old disk population runaway star. 4.2 - 4.24v. Binary with HR 4678. Binary with HR 4677. Companion G8III, optical. Delta Sct 6.40 - 6.48V, 0.05515028d. Also possible cycles of 0.0713d. The first Delta Sct type star to be discovered in a galactic cluster. FM Com4.9, 5.4, sep. 0.008". Also astrometric and interferometric double, 5.4v sep. 0.124", position angle changed 35d in 1.5yrs. Delta Sct? ZaniahPrimary may be close double 5.8, 5.8v, sep. 0.6". Visual companion 11.6v at 132". Companion F6III optical. CPM. Companion also dF2. I? 3.4 - 4.0v. AC binary. C, 8.55V, +0.52(B-V), +0.01(U-B), F7V. Component B, 12.52v at 35" optical. Binary. Secondary is dK5. ADS 8531B, 8.0 - 9.5V. Delta Sct 5.89 - 6.15V. Multiple periods 0.2085, 0.1529, 0.1259 and 0.1158d. AI CVnE? Amp. 0.067V. Alpha CV 5.18 - 5.20V, >1d. GN ComComponents K3IIIab and F8IV. AB 6.76 A7V, 7.79 F4V, 678.0y, a = 1.30". AB 1.35 B0.5IV, 1.75 B3n or B0.5Vn, q = 0.916". Mag. and colors for blend of HR 4730-31, 0.76V, -0.25(B-V), -1.00(U-B), -0.24(R-I). Masses 14 and 10 solar for hyperbolic orbit with periastron distance 61 AU. Possibly X-ray source 2U1223-62. Acrux is a bright binary star system whose combined light makes Acrux the 14th brightest star in the sky. It is about 400 [G/light system is much larger than our [G/Sun] (14 and 10 solar masses respectively). ACRUXIn stage of rapid evolution after core hydrogen exhaustion. Faint CPM at 542" S. prec. Amp. 0.35V, 0.25p. BL CruDelta Sct 6.20 - 6.23V, 0.05d. Form of light curve varies. FT VirCPM with HR 4752. Component C, 14.7V at 2" from B. CPM with HR 4751. Alpha CV + Delta Sct 5.23 - 5.40V, 5.0633 or 5.0754d and possible pulsation 0.052d. Var. magnetic field UII varies with period 71 min. AI ComCPM. B is K2Ve, lithium strong. ADS 8572A. AlgorabAB 6.5 G0V, 8.6, 161.53y, a = 1.385". I? Amp. 0.30p. GacruxLb? 4.95 - 5.04V. CQ DraAlpha CV + Delta Sct 5.41 - 5.46V, 2.1953d with secondary variations of 1.0256d and 0.9178d. Also Delta Sct amp. about 0.01V, 0.0227d or 0.0274d and 0.2909d. Considerable discordance among observers. CaII and SrII vary in period about 1d; period changes. UU ComCDelta 5.36 - 5.58V, 3.34258d. BG CruDelta Sct? Probable nearby star. Beta CVn amp. 0.05V. Chara is the namKraz in BecvarRadio star. Gamma Cas 3.82 - 4.10V. H alpha and H beta emission vary period about 30d. H alpha profile changes in 1 min. or less. Binary with HR 4792. Binary with HR 4791. 5.11 - 5.16V. Delta Sct, amp. 0.02B, 0.082d. TU CrvCompanion B4V, optical. Beta C 2.68 - 2.73V, 2.17 - 2.24p, 0.0903d. CPM? Combined mag., colors. Companion B7p. H alpha emission var. 0.1V, 0.15d. FW VirEll? Amp. 0.025V, 0.58:d. FH MusAlpha CV 6.32 - 6.55V, 4900:d. AX CVnAlpha CV? 4.61 - 4.66V. Period about 0.46d: AB 2.9 A0III, 2.9 A0III, 84.50y, a = 0.930". Combined mag., colors. CDelta 5.89 - 6.49V, 7.510211d. Period changes. R MusBinary with HR 4822, q.v. See HR 4822. EA? 4.91 - >7.5V, 5.0 - >7.5p. Faint May 22, 1896. Also amp. 0.04V suspected on time scale 1d. Delta Sct, amp. 0.02U,B,V; 0.056 and 0.042d. GG VirBinary with HR 4825, q.v. Delta Sct? Amp. 0.02V, cycles 0.02 to 0.10d. Gamma Cas 5.24 - 5.45V. BZ CruAmp. 0.07V. 3.7 B2V, 4.0 B3V, 383.12y, a = 1.735". Combined mag., colors. SRb 7.4 - 10.0p, 158.0d, some cycles 250 and 90d. Possible secondary 2000 - 2200d. Y CVnDelta Sct 5.20 - 5.23V, 0.0756d. FM VirProbably optical. CPM? Companion A3p. Comp. B, 8.70 - 8.82V, Ap. Possible spectrum var. Interferometer measures indicate close double or multiple star. Component B, 11.4v, F8V, optical; C, 7.5v, B8. Beta C 1.23 - 1.31V, multiple periods, 0.2365072d, 0.160474d, 0.121383d, 6d, 7 - 8y and others. BecruxAlpha CV 6.29 - 6.39V, 16.31d. Same rotation period. Var. spectral lines and magnetic field. Magnetic and rotation axes nearly aligned. EP VirAmp. 0.05V. Optical. Equal components. Delta Sct? 5.9 - 5.94v. B, optical. Amp. 0.07V. H alpha emission var. Suspected occultation double. CPM with HR 4893. CPM with HR 4892. AB 5.05 G8III, 7.22 F3V, 510y, a = 1.42", or 674.23y, a = 1.897"; masses 2.7 and 1.4 solar. Component C, 9.74V, +0.73(B-V), +0.31(U-B) G3IV-V 29", possibly physical, although a hyperbolic orbit has been computed with periastron about 400 years ago. CDelta 6.23 - 6.92V, 4.68997d. S CruBeta C?, amp. 0.02V, 0.3951d, possible secondary 0.1793d. CPM with HR 4899. CPM with HR 4898. Gamma Cas 4.99 - 5.18V. Mu2 CruCombined mag., color, 6.7, 6.8v, sep. 0.100"; occultation double. Close binary, sep. 0.040", unresolved by speckle interferometry. If companion on main sequence, the inferred spectral type is F6V. Lb 4.7 - 4.8V. Alpha CV 1.76 - 1.79V, 5.0887d. Spectrum variable. Photometric var. due to UV absorption from overabundant metals. ALIOTHCompanion K0III. SRb 5.55 - 6.6V, 7.2 - 7.7p, 50d. TU CVnAuvaCep-like supergiant, 6.61 - 6.69V, amp. 0.32B, 43.96d preferred; 53.33 or 67.80d also possible. LN HyaBinary with HR 4915. Binary with HR 4914. ADS 8706A, Alpha CV 2.84 - 2.98V, 2.78 - 2.81B, 5.46939d. The prototype star. Var. magnetic field with same rotation period. COR CAROLIAB binary? C, 10.4v at 124" optical? CPM. Component A suspected occultation double. CPM. AB CPM. C, 13v at 36" optical. ADS 8732B, 8.0 - 11.0v. BC, 9.5, 9.9v sep. 2". AxBC optical. 6.02 - 6.17V. Miscellaneous magnitude determinations range from 5.93 to 6.132V, probably confirming variability. Also suspect amp. 0.03V on time scale 2 hrs. 5.05 F2V, 7.43 G6V, 109.97y, a = 1.270" or 106.7y, a = 1.281". Combined mag., colors. ADS 8739B, 7.5 - 10.5v. VINDEMIATRIXCPM? Combined mag., colors. Lb? 7.9 - 8.01p, amp. 0.09V. V789 Cen8.1 - 8.20B. Companion K0Ve, high lithium abundance. CPM companion F7V. 5.1 - 5.3v. Period of some hours? AB CPM. BC, 11.9, 12.1 sep. 0.4" in 1901, single in 1958. Companion at 149" from A, noted by John Herschel, small nebula. SRb 5.30 - 6.1v, 58:d. FS ComCPM. vsini of secondary 110k/s. Second brightest Wolf-Rayet star in the sky. E + WR 5.50 - 5.52V, 18.341d; UV, var. 1.5d. A is SB and speckle interferometric binary, third component 9.4v, sep. 7.1". B, 8.00V, +0.20(B-V), -0.09(U-B), CPM. Alpha CV, amp. 0.035V, 1.272d. V824 CenADS 8805BC. Binary? C, 11.2 at 1". A is HR 4971, not CPM. ADS and IDS differ on naming of the components. IDS, adopted here, is the more consistent with FGW Struve's early discovery. AB 5.05 F5V, 5.08 F5V, 25.87y, a = 0.662". Colors, spectrum for combined light. Mag. of blended HR 4968, 4969 is 4.32V. ADS 8804A speckle interferometric sep. 0.43" 1978.40, 0.58" 1981.47. Var. of combined light with HR 4969 not confirmed, but 90d inclination of orbit indicates eclipses possible. DiademAB 5.0 B8V, 5.7 B9V, 27.0y, a = 0.185". Combined mag., colors. C, 8.4v at 2" physical. 4.54 - 4.65V, combined light of 5.2, 5.8, sep. 0.3". Uncertain which component is variable. V831 Cen7.2 A5V, 7.3 A5V, 19.0y, a = 0.118". Combined mag., color. B, 12.5v at 79". Component C at 184" discovered by John Herschel in 1897 not seen 1908 or later. Binary. Component B, 8.2 A0p, Am?, CPM. E? 4.76 - 4.81V. Optical. 6.54 - 6.60p. Delta Sct 6.67 - 6.72V, 0.119153d. Probably long beat period; long intervals const. mag. DK VirFainter component 8.5 - 10.5v. Companion is GC 17977, 8.2v A2, CPM. 4.8 - 4.85V. Delta Sct 4.70 - 4.75V, 0.12168d. Var. amp.? AO CVnAlpha CV, amp. 0.04V, 0.767d. BK CVnAmp. 0.10V. Possibly double. Old disk population runaway star. Amp. 0.10V. Aa = AP 3.0 A2V, 3.0 A2V, sep. 0.0115", 0.056y, a = 0.012". Combined mag., colors AP. Binary with HR 5055. Alcor, HR 5062, at 709", CPM. MIZARSpica is the 16th brightest star in the sky. It is a binary star system that lies 142 [G/light year]s away. The largest of the two stars is almost 11 times more massive than the [G/Sun], while the second star is approximately 7 times the mass of our star. Interferometer indicates visual component A is multiple system. Occultations yield three companions: 3.1v at 0.0025", 4.5 at 0.05" and 7.5 at 0.5". Combined mag. and colors. Visual component B, 12.0v at 148". Ell (Beta C) 0.97 - 1.04V, 4.01454d, and Beta C, 0.1737853d. Period changes. SPICAComp. A is speckle interferometric binary, sep. 0.045". CPM with HR 5054-5. Delta Sct. ALCORAlpha CV, amp. 0.09V, 4.3127d; alternative periods 4.3032, 4.3224d. EZ MusFirst known potassium flare star. CPM with HR 5075. CPM with HR 5074. ADS 8920A, M 3.5 - 10.9v, 388.87d. Period varies; was 500d beginning of 18th century. M8 at minimum. Discovered by Montanari in 1670. R HyaComponent B is CPD -76d769. CPM. Cst 6.6p. S ChaBinary. 4.5 G8III, 4.7 G9III, 78.7y, a = 0.165". Combined mag., colors. Unresolved by speckle interferometry. HX VirAlpha CV 4.91 - 4.99V, 3.7220d, also magnetic field and rotation period. Probable irregular magnetic variable. CW VirAB 6.5 A1, 6.9, 197.7y, a = 0.563". C, 12v at 26" optical. ADS 8954. Uncertain which, if either, A or B varies. HezeOptical. RS 4.94 - 5.01V, 2.6131738d. Probable reflection effect. BH CVnDelta Sct? AB 6.2 F6V, 6.5, 34.969y, a = 0.463". Combined mag., color. Companion 8.5v F6V, CPM. AB binary. B is A7IV. AB 5.01 A7III, 6.91 F0V, 240.0y, a = 1.091" or 220.4y, a = 1.205". Combined mag., colors. Companion B1p, optical. Beta C 2.30 - 2.31V, 0.169608, 0.17696 or 0.2150d. Multi-periodic. Binary. Companion K3III. SRb 5.14 - 6.55V, about 90d. Amp. 1.2V, 0.19(B-V), 0.47(U-B) from another source. Possible type E with very long period. V744 CenLb? Amp. 0.08V. V765 CenAB 6.3 F0IV, 6.3 F2IV, 22.35y, a = 0.208". Combined mag., colors. Masses 7 and 6 solar. AB binary. B is Am. AB combined mag., colors. SRa 5.5 - 9.0v, 90.44d. Amp. 2.04V, 0.32(B-V), 1.09(U-B). Spectrum variable. T CenCPM. Alpha CV 6.24 - 6.26V, 2.449909+/-0.000011d, asymmetric light curve. Spectrum var. CQ UMaVariations in 17 and 24 min., amp. about 0.8B. Third component 9.2v at 0.8" from A. Alpha CV, amp. 0.025V, 2.605d. V827 CenBinary. B = NSV 6401. ADS 9000B. Delta Sct? Amp. 0.02V. Visual companion 11.7v at 44". Primary is occultation triple, companions 8.2v at 0.039" and 8.4 at 0.061". Companion 10.01V, +0.78(B-V). One of the intrinsically most luminous stars in the Galaxy. S Dor? 6.17 - 7.50V. V766 CenAB CPM. CD at 27", 11.9, 13.1v sep. 2", binary. High space velocity. Amp. 0.08V. CPM with +7d2692, 9.4v at 486". Binary, period several centuries. Companion M2. Delta Sct? 4.40 - 4.58V. Alpha CV 5.64 - 5.67V, 1.37996d, amp. 0.03U. Spectrum variable. CR UMaCPM. Beta C?, 3.40 - 3.43V, 3.48 - 3.52R, 0.175d. Alkaid is located at the end of the [G/Big Dipper]'s handle. It is about 93 [G/light year]s distant. ALKAIDSRb 4.16 - 4.26V, 5.79 - 5.87P, 12:d. V806 CenCompanion F2V, optical. Gamma Cas 2.92 - 3.43V, 3.535d. Variable H alpha. Expanding circumstellar shell. R and I mags. decreased by about 0.3m between 1965 and 1983. Variable line profiles. CPM. Companion 7.72V F0Vp. See HR 5210. SR? 4.72 - 4.81V. AW CVnVisual companion, 8.35V, +0.36(B-V), +0.12(U-B), A3Vm, vsini 71k/s. AB 6.3 F2, 6.5, 257.7y, a = 1.268". Mag., colors for combined light. Component E, 8.5v at 66" optical. Companion B8V. Gamma Cas 5.85 - 6.26V. H alpha also variable. V767 CenLb? 4.52 - 4.67V. CU DraExpanding circumstellar shell. ADS 9053, 2613y, a = 4.998". A* 2.68 G0IV. Visual component 8.8v at 113" optical. MufridI 6.1 - 6.6p. Expanding circumstellar shell. SRb 6.4 - 8.6p, 119d. Amp. 0.56V, 0.10(B-V), 0.26(U-B). IUE observations on Aug. 2, 1985 and Oct. 2, 1986 show slight increase in visual mag. and decrease by 0.9 mag. in Mg II 2800. B is G type, optical. Hadar, a bright, hot star, is the 10th brightest star in the sky. It is over 360 [G/light year]s away and has a companion star that is difficult to see with a small telescope. Beta C? Amp. 0.07V, 0.157d, modulation 352d. Line profiles also vary per. 0.157d. HADARAlpha CV, amp. 0.045V, 1.837d. V828 CenA*, 9.897y, a = 0.1075". Unresolved by speckle interferometry 1986.45. Amp. 0.04V. Amp. 0.020B, 0.035d. MenkentThuban is the bright star located halfway between the bowl of the [G/Little Dipper] and the second star of the handle of the [G/Big Dipper]. It is approximately 180 [G/light year]s distant and 135 times more [G/luminous] than our [G/Sun]. 4,800 years ago, Thuban was aligned with Earth's North [G/Celestial Pole], making it our North Star. Alpha CV?, 3.64 - 3.67V. THUBANCompanion K2V. Companion K2. Amp. 0.08V, 1.456d. Suspected occultation binary. Lb? 4.98 - 5.33V. BY BooLb 5.2 - 5.3v, 7.0 - 7.13p. CF BooSRb 4.80 - 5.00V, 80d. ET VirPossible runaway star. EB 5.96 - 6.52V, 1.49009305d. V716 CenOptical companion. Alpha CV 4.98 - 5.05V, 0.52067688d. Same period spectrum var. Si a major source of photometric variability and suggests starspots related to magnetic field. SiII varies out of phase with HeI. Period unusually short for star with peculiar A-type spectrum. CU VirComponent B, M3IV; C, F4V; both optical. Gamma Cas 4.97 - 5.10V. V795 CenDelta Sct amp. >0.05B, over 2 hrs. Companion F5V, optical? I 1240A, M 5.3 - 11.8v, 546.2d. R CenBinary with HR 5329. ADS 9173B. Formerly suspected amp. 0.01V, not confirmed. Binary with HR 5328. ADS 9173A, Delta Sct 4.50 - 4.58V, 0.06682 or 0.076242d. Possible beat period of about 16d. Asellus TertiusLb? 6.37 - 6.52V. FS Vir4.06 - 4.11V. SyrmaArcturus is the fourth brightest star in the sky. It is 25 times the diameter of our [G/Sun] and 115 times more [G/luminous]. It is only 37 [G/light year]s away. High space velocity? H and K emission vary. ARCTURUSAB CPM? B is K0V. Delta Sct 4.73 - 4.78V, amp. 0.025B, about 40 min. Asellus SecondusAlpha CV 5.73 - 5.93V, 9.29477d. Line intensities, rotation and magnetic field same period. Also possible magnetic cycles about 1 hr. CS VirAB CPM. B, 13.3v at 3". Combined mag., colors. Occultation sep. 0.006", mag. diff. 1.4B. Possibly triple star with SB. Optical. AB binary. Component A is close double, sep. 0.2", combined mag. and colors. SX Ari 4.38 - 4.43V, 8.814d for light, He, magnetic field; light and mag. field max. correspond to He min. Sp. from B2V to B7IV in per. 8.8172d. Var. possibly due to rotation of inhomogeneous surface; possibly prolate spheroid. V761 CenBC 7.5 F0V, 7.6 F2V, 39.50y, a = 0.228". Combined mag., colors. Also binary with HR 5386 = ADS 9247A. EA? 5.7 - 6.2p. Beta C 4.54 - 4.58V, 4.36 - 4.43B, 4.10 - 4.14p, 0.17738884d. Binary. Combined mag., colors. Triple system. BC, 7.0v A4V or A1IV, 8.2v sep. 1". vsini of B is 60k/s. CPM. Asellus PrimusABxC, CPM. C, 10.0v at 4". AB binary. Combined mag., colors. Companion G6Ve, optical. Fixed with HR 5414. CDelta 6.43 - 7.21V, 5.493839d. V CenCompanion K1V. Identification of companion questioned. Component C optical. 6.5 A7IV-V, 6.7 A7IV-V, 30.0y, a = 0.210". Combined mag., colors. Primary found double by speckle interferometry, sep. 0.069". Component B, optical. Delta Sct 3.02 - 3.07V, 3.23 - 3.28B, 3.20 - 3.25p, 0.2903137d. Hydrogen and Ca lines vary. SeginusCompanion K0V. Innes catalogue indicated a faint companion at 6" in 1897, not subsequently seen. Gamma Cas 2.30 - 2.41V, 1.83 - 1.95p. H alpha variable, H beta sometimes bright, sometimes dark and double or multiple. Variability shows evidence of mass loss. Amp. 0.07V on time scale 1d suspected. Delta Sct? Amp. 0.02V, over 3 hours. CP Boo5.52 - 5.56V. Delta Sct? AB combined mag., colors. C, 9.2A1V at 19" = CoD -45d9303, CPM? Lb, amp. 0.14V, 7.2 - 7.34p. CH BooS, amp. 0.1:V, 0.20U. Expanding circumstellar shell. AB 79.920y, a = 17.515". B = HR 5460, CPM with Proxima at 2.2d, discovered by Innes in 1915, a flare star, V 645 Cen, 12.4 - 13.4p, 11.10V, +1.88(B-V), +2.05(R-I), M5.5Ve. RIGEL KENTAURUSSee HR 5459. Binary. Companion K5V. Amp. 0.03V. Magnetic var., about 4 months. Pulsation period 6.8 min? Beta C 2.29 - 2.34V, 0.2598466d. Period varies. Possible secondary period 3.145d. Modulation period 10y? Possible nearby star on basis of spectroscopic parallax. Binary with HR 5476. Colors for combined light. Mag. for blend, 4.53V. ADS 9338A, Alpha CV? 4.94 - 5.00V. Binary with HR 5478, q.v. H alpha variable. Rijl al AwwaBeta C, amp. 0.04u, 0.03y, 0.04V, 0.131d with possible secondary periods. BU CirSRb 4.7 - 5.4v, about 30d or 450:d. W BooDelta Sct 6.47 - 6.52V, 0.08d. BP OctBinary. Delta Sct 6.22 - 6.29V, 0.0825 and 0.0837d. Difference in mag. between components of double varies. DL DraBinary, components F0V, G1V. 7.0 F7V, 7.2, 25.95y, a = 0.297". Binary with HR 5505. Colors for combined light. Mag. of blend, 2.37V. IZARSRb 5.93 - 6.15V, 60 - 80d? V768 CenCPM? AB and AE binary. B = Am(A2/A6/A8)s. C and D optical. E 12.5v at 27". ADS 9396AB, Alpha CV. In Innes catalogue, 6.5, 6.5v sep. 0.5" in 1913. Not confirmed. CDelta 5.65 - 6.09V, 5.273268d. AX CirBinary. CPM with HR 5531 at 231". Component A, HR 5531, is the suspected occultation double, 3.4, 3.8, sep. 0.01". CPM with HR 5530. Suspected occultation double. Zuben ElgenubiMergaAB binary, B is G7V. Binary. Combined mag., color. Cst? 7.8p. R ApsAB 4.74 G8V, 6.9 K4V, 151.505y, a = 4.904". Combined mag., colors. Masses 0.89 and 0.74 solar. Perturbation period 2.2y, a = 0.020" suspected; unresolved by speckle interferometry. Component C optical. BY? 4.52 - 4.67V, 10.137d. B, 10.8v at 13", CPM. 6.8 F4IV, 7.5 G1IV, 215.4y, a = 1.09". Combined mag. Gamma Cas 5.02 - 5.44V. Amp. 0.03 on time scale 2d reported. H alpha varies. CPM? Combined mag., colors. KOCABAB 5.79 K4V, 7.93 M2V, q = 20.388" hyperbolic orbit. Component B is dM2. CPM. 2.9 - 2.95B. 6.3 A4V, 6.6 A6V, 339.3y, a = 0.93". Combined mag., colors. AB CPM. B is G8V. CPM. Companion M1. EA 4.92 - 5.90V, 2.32735297d, period may vary. Component A of quadruple system. Contact binary. Zuben ElakribiSR? 6.17 - 6.5p, 40?d. RR UMiAB CPM. Component C, 14v at 32" optical. CPM. Component B F4V. ADS 9447A, Alpha CV 6.33 - 6.41V, 0.6080722 or 0.741285 or 2.8881d. Magnetic field var. 0.7447d?, possibly irregular. BX BooNekkarSRb 3.20 - 3.46V, 20d. BrachiumLb? 6.38 - 6.46V. GM LupBinary with HR 5606. Colors for combined light. Blended mag. 3.88V. vsini for combined light. 5.3 F5V, var. G2V+G2V, 225.0y, a = 3.772". Combined mag., colors. Combined mass 2.1 solar. ADS 9494B, EW 6.5 - 7.10v, 0.2678160d. Period changes with orbital motion. Variation in light curve may be caused by mass transfer between close pair. Reddening at max. due to ADS 9494A. Component A may vary up to 0.09m. i BooSpectrum variable. Amp. 0.09V. Alpha CV 5.76 - 5.81V, 0.8775d. HR Lup4.6 B3V, 4.9 B3V, 72.88y, a = 0.422". Combined mag., colors. CPM. Companion A5. 6.7 A2V, 6.8 A1V, sep. 0.08", 8.0y, a = 0.10". Combined mag., colors. Unresolved by speckle interferometry. Both companions optical. IUE observations show a B8V companion 2.5 mag. fainter than primary. Optical pair with HR 5643. Lb 8.1 - 9.1p. Amp. 0.51V, 0.36(B-V). X TrACPM with HR 5647. See HR 5646. CPM. B is F8. Nearly same proper motion as HR 5646, 5647. Var? Amp. 0.015b. AP 5.1 B9IV, 5.6 B9V, 23.42y, a = 0.116", combined light, colors. Mean mass 5 solar. BC, 10.5, 11.2v sep. 1.9". A physical pair in orbital motion about AP at 58"; possibly quintuple system. ADS 9532A, Alpha CV?, 4.53 - 4.56V. Spectrum variable. Resolved by speckle interferometry 1986.45, sep. 0.51". Lb 5.79 - 6.02V. FL Ser7.1, 7.1v, sep. 0.03"; suspected SB, but duplicity doubtful. Binary. Companion 7.53V, +0.35(R-I), dG6. Component C, A5V, optical. Component B, RV -16k/s. CPM with HR 5664. CPM with the triple star HR 5661. Faint companion of HR 5664, G5V, probably optical. Component A of double, Ell?, amp. 0.08V. Suspected of being double. SKYLAB indicates cool star with hot companion. Companions: B, B9V; C, A-type spectrum. CPM. AB binary. C, 7.17V at 23" CPM. Described by Eratosthenes (ca. 200 B.C.) as brighter than Antares, by Ptolemy (ca. 150 A.D.) as equal to Antares. Zuben ElschemaliEB 5.49 - 6.0B, 2.164175d. Period 1.85 found for secondary min. GG LupAB binary. Some disagreement as to whether B or C, at 127" from A, is the brighter. MQ SerBeta C 3.21 - 3.24V, 0.16547d; 0.14273d also possible. Probable CPM. 5.1 B5, 5.5 F8, 778.54y, a = 2.384" or 269.90y, a = 2.485". Although a period has been derived, spectroscopic evidence indicates that the F8 component is a dwarf much closer to the Sun than the B5 star: probably optical. AB binary. Combined mag., colors. C, 9v at 27" probably optical. Var? Amp. 0.015b. CPM? Pherkad MinorSpectrum variable. AB 5.62 G1V, 5.89 G3V, 41.623y, a = 0.907". B is HR 5728. Colors for combined images. Mag. for blend 4.98V. Masses 0.95 and 0.94 solar. C, 13.4v at 58" optical; D, 11v at 215" probably optical. Blend of 5727/8, 4.94 - 5.02V. Uncertain which component is the variable. Companion K5IV. Gamma Cas 5.43 - 5.61V. If variable, period much longer than 180d. Probably binary with HR 5734, a close binary ADS 9626BC. Delta Sct? AlkaluropsBC 6.98 dG5, 7.63, 260.10y, a = 1.463". Combined mag., colors of BC. Mean mass BC, 0.52 solar. Delta Sct? Amp. 0.03V. Hydrogen and CaII variable. PherkadPossible nearby star on basis of spectroscopic parallax. Zeta1 Fl 32Ed AsichFirst astrometric binary discovered from parallax measurements, by K. Burns, 1931. Alpha CV 3.65 - 3.72V, 18.487d. Magnetic field and rotation same period. Variable H alpha. Amp., light, magnetic field, spectrum vary per. 10.5y. Possible secondary light period of 240d. NusakanB, 8.94V, +0.55(B-V), +0.07(U-B), F6V or G0V, CPM at 11.2". A, doubtful occultation double, mag. and color combined, sep. 0.03". BC 7.8, 8.0, combined F0V 54.3y, a = 0.225" or 57.32y, a = 0.245". This pair binary about component A at 9.3". Companion A5. Combined mag., colors. Companion resolved by speckle interferometry, sep. 0.040" on 1985.5. 3.5 B2IV-V, 3.6 B2IV-V, 147y, a = 0.59". Combined mag., colors. Component A is NSV 7134, 4.12V, amp. 0.7m. However, 1300 UBV observations on 57 nights (1984-6) revealed no variation over 0.06 mag. R-I also found at -0.16. Component B, the rarely seen companion, is NSV 7135, 5.5, 7.8v. Var? Amp. 0.015b. Companion B, K0V; C is optical. ADS 9704 AP, sep. 0.097", unresolved by speckle interferometry. Component B, 11.2v at 42", optical. Zuben ElakrabADS 9701, 3168y, a = 5.8432". Binary with HR 5789, blended mag., colors. Alphekka is the brightest star in [X/Corona Borealis]. It lies approximately 75 [G/light year]s distant and is about 45 times more [G/luminous] than our [G/Sun]. EA 2.21 - 2.32B, 17.359907d. Possibly also intrinsic var. ALPHEKKACPM. Binary with HR 5816. Binary with HR 5815. Combined mag. 5.79V. AB binary, B, 8.5 G8IV-V; C, 11.4 at 135". Companion 10.33V, +0.49(B-V), -0.01(U-B), F5V, CPM. Binary with HR 5833. Is 7.3 - 8.3p. AB 5.2 A1V, 5.3 AIV, 11.07y, a = 0.117". AB combined mag., color. Resolved by speckle interferometry 1986.45, sep. 0.05". Alpha CV 5.33 - 5.36V, 1.59584d. SrII same period. Magnetic field var. Period probably due to rotation of star spots. CPM. 4.08 A0IV, 5.51 A3V, 91.0y, a = 0.74". Combined mag., color. Delta Sct 3.80-3.86V, 0.030d. Mass 1.9 solar. Possibly beat period? CPM with HR 5851. Quintuple system of which E is brightest companion; B, 12.0V at 4"; others at 172" and 208". SR? Amp. 0.2V. ADS 9765B, optical. UNUKALHAIAB binary; C, 9.0 G0 at 51" fixed. Alpha CV 5.50 - 5.51V, 1.30488d. Beat period 4.2283d. BP BooSep. 0.097". AB, CPM. B, 9.72V, +0.84(B-V), +0.68(U-B), K3V, CPM. C, 10.7v at 201". Also CPM with BD+15d2906 at 1642", itself a double, 8.4, 10.5v sep. 6". Component B, K0V. Third component optical. R CB 5.8 - 14.8v. The prototype star, discovered by Pigott in 1795. R CrBComponents white and orange-red. Amp. 0.07V. B, 10.5v at 1.08"; C, 9.1 at 45"; D, 8.7 at 48". Amp. 0.07V. Binary. Delta Sct? CPM. Combined mag., color. Suspected occultation double. Amp. 0.03V on time scale 2 hrs. suspected. 1.45937d. Magnetic field variable 1.45955d (Landstreet et al. 1979, MNRAS, 188, 609). V927 ScoVariable intrinsic polarization observed Aug. 1974. Binary. Companion G8V, optical. Delta Sct 6.20 - 6.23V, about 0.250d. FP SerCompanion F5V, optical. High space velocity. Binary with HR 5926. Mag. and color for combined light, 4.585V, +0.09(B-V), +0.07(U-B). Binary with HR 5925. Suspected occultation double. Old disk population runaway star. Companions optical? Beta C?, 5.84 - 5.87V, 0.2872d. Spectrum var. Balmer emission and metallic absorption vary in period about 30 yrs; H alpha profile varies in period of =<1 min. A potassium flare observed June 21, 1965. Probable mass-transfer between components. CDelta 6.06 - 6.81V, 6.32344d. Possible blue companion. S TrAGamma Cas 4.79 - 4.96V. Variable polarization. R-I also found at -0.13. FX LibSmall amp. in y. 0.492d or 0.976d. Also spectrum var. V913 ScoPrimary is SB, 3.4, 6.4v sep. 0.0003"; third component, ADS 9862B, 12.2v at 50". vsini both A and B =<100k/s. Component B, F4V, optical. Component B, 12.6v at 2", CPM. Possible X-ray source 3U1555+27. AB binary. Companion A5Vp. Possible quadruple system: SB 3.0, 5.0v, sep. 0.00001", 3.3v at 0.1", and 4.9v at 0.186". DschubbaComponent B optical. Delta Sct 4.95 - 5.00V, 0.063d. CL DraAB 5.3 A5V, 5.5 A6V, 26.93y, a = 0.366". C, 7.5v at 11". Combined mag., colors. Companion optical. Alpha CV?, 4.96 - 5.08V. Binary with HR 5978, q.v. CPM with HR 5985 = ADS 9913C, at 14" and with B, 5.9v at 0.5", possibly SB. Lunar occultations and speckle interferometry indicate companions 4.2v at 0.001" from A and 7.6v at 0.129" from C. Occultations by Jupiter and Io in 1971 indicate complex system. Component C occulted by Io revealed the 2.5 mag. fainter companion at 0.1". GraffiasCPM with HR 5984, q.v. Spectrum var., amp. 0.03V, 1.49187d. V929 ScoAB binary, B, 9.2v at 1"; C, 10.4 at 29" fixed; and D, 10.8 at 53" optical. Amp. 0.02(b-y). CPM with HR 6000 at 44". CD, 7.1, 11.7v, sep. 1.3". 6.97 - 7.71V, about 30d, variability attributed to circumstellar dust. Possibly a binary shell star with mass exchange. Considerable confusion between HR 5999 and 6000 particularly as to which is the variable and which the brighter. Originally announced as HR 6000, V856 Sco is really HR 5999, the southern preceding and fainter component C of the bright double. The error stems from interchanged photometric data in Harvard Annals 45, 197, 1901, all other early visual and photographic estimates indicating that the S. prec. component is the fainter. V856 ScoCPM with HR 5999. Component B, 13v at 298". Not the variable. Originally confused with HR 5999. CPM. Components K0.5IIIab and F4III. Optical pair with HR 6009. MarfikOptical pair with HR 6008. Amp. 0.04V. FS SerCPM. Physical pair with HR 6021. Lb? 4.66 - 4.87V. Physical pair with HR 6020. Amp. 0.13V. Alpha CV?, 4.23 - 4.27V, amp. 0.015U, 7.832d, symmetric light curve. ADS 9951A is SB, 4.9, 6.9v, sep. 0.0003". AB, binary. Component B, 6.9v at 1". Components CD at 41" = HR 6026, q.v. HR 6026, q.v. JabbahBinary, companion F3V. A5, F1. Binary. Lb? 5.58 - 5.83V, 7.1 - 7.31p. LQ HerAB binary. C, 10.5v at 78". Sep. 0.090". Companion, 10.73V, +0.58(B-V), +0.08(U-V), F8IV:, CPM. Sep. 0.03". Amp. 0.10V. Yed PriorOptical. CDelta 6.12 - 6.77V, 9.75411d. Period changes. Possibly blue companion. S NorBinary with HR 6063, q.v. A4, A7. Yed PosteriorCompanion, F9V, CPM. Small amp. in V. MgII 4481 appears to vary. B, 8.26V, +0.25(B-V), -0.23(U-B), B9.5V at 20", optical; vsini : 54k/s. The visual primary is triple: SB, 3.3, 5.3v, sep. 0.0005" and 5.5v at 0.49", discovered by occultation. Beta C 2.94 - 3.06B. Multiple periods, 0.2468429, 0.239671, 8.2, and 33.1d. Surrounded by HII region. Primary period varies in period of 23.2y with an amp. of 0.7 sec. Occultations indicate the variable has a 2.2 mag. fainter companion at 0".49. The duplicity had been suspected from occultations as early as 1860. Orbital period probably over 112 yrs. UV observations indicate temperature varies by 2510K and ratio max. to min. radius by 1.095. AlniyatCPM. Lb 6.8 - 7.5p. AT DraCPM. ADS 10010AB, 6700y. 3.85 - 3.90V. Amp. 0.07V. ADS 10022B, 9.58v, optical. Components also classified B9.5V(n) and A1V(n). Sep. 0.098". Binary with HR 6105. Mag. and colors for combined light, 5.41V, +0.59(B-V), +0.12(U-B). Visual companion, 9.76V, +0.87(B-V), +0.43, G7IV:. See HR 6112. Companion 7.46v B9V, CPM, possibly binary with the SB. B, 12.0v at 2" CPM; C optical. Alpha CV, amp. 0.08V, 2.951d, double wave light curve. Also rapid var. 0.15d. KajamGamma Cas 4.18 - 5.0V. Long term variation in emission lines. Variable polarization. R-I also found at +0.09 and +0.11. E, amp. 0.017V, 2.144202d. DQ DraHigh space velocity. SRb 5.0 - 5.38V. V2105 OphComponent B of visual double, 7.0 - >11.0v. Binary. Companion gG7. Gamma Cas 5.29 - 5.41V. QU NorADS 10058A, var. suspect NSV 7713; ADS 10058B, var. suspect NSV 7712, 8.8v, dK2, amp. about 2v. This bright red supergiant star has a diameter of 600 million miles (1,000 million km), making it almost 700 times larger than our [G/Sun]. This star is in its final stages of life. Once it has used up all the fuel in its core, Antares, will explode in a [G/supernova] explosion. What's left of the star will form either a [G/pulsar] or a [G/black hole]. Antares is 135 [G/light year]s away. Var. M1Ib, 5.5 B2.5V, 878y, a = 2.90", masses 15.5 and 7.0 solar. Companion is radio source. SKYLAB confirms cool star, hot companion. ADS 10074A, SRc 0.88 - 1.8V, 1733d. Possibly considerably fainter before 150 A.D.: see HR 5685. ANTARESAB binary. Components A (F5V) and B both optical. Spectrum variable? SRb 4.3 - 6.3v, 5.7 - 7.2p, 89.2d. Also slow var. of about 875d and aperiodic superposed cycles 5 - 15d. g HerVisual companion probably optical. KornephorosAB 4.16 A1V, 5.22 A4V. 129.87y, a = 0.970" or 126.78y, a = 0.95", combined mag., colors. Component C, 11.0v, 120" CPM. MarficAlpha CV, 4.45 - 4.51V, 1.79 or 4.67d. Alpha Cyg? 4.87 - 4.98V. 4.82 - 4.85V. Amp. 0.08V. V918 ScoSep. 0.067". Noted as double by speckle interferometry in 1971-2, unresolved at Mayall 4-meter in 1976. Spectrum double-lined. Resolved by speckle observations 1986.45 (Blazit et al. 1987, A&AS, 71, 57). Companion A2V, CPM; vsini 80k/s. Amp. 0.04: at wavelength 4530; 0.02: at 6585. Rotation period from starspots, 11d. V2133 OphCPM. COPERNICUS observations of CO indicate a SN remnant near Zeta Oph which may have caused Zeta Oph to become a runaway star. Gamma Cas 2.56 - 2.58V. Spectrum var.: UV spectra in 1972 indicated mass outflow probably related to formation of shell. Evidence disappeared in 1974. H alpha in absorption 1971, emission 1973. Rotational period 19.7 hrs. Alpha CV, amp. 0.03U, 0.02B, 0.01V, 1.45876d. V773 HerSep. AB, 0.102". About 6d. Spectrum variable. CPM with HR 6185. Binary with HR 6185, q.v. AB binary, 5.6, 9.0v sep. 1.6". C = HD 150135, O7:, CPM. Binary with HR 6195. Component B is speckle binary, sep. 0.145". Component C, optical. A companion 0.145" from B discovered by speckle interferometry. Binary with HR 6194, q.v. Optical. Amp. 0.05v, 3.76d. LP TrACPM with HR 6209 at 96". CPM with HR 6206. ADS 10157AB, 2.90 F9IV, 5.53 G7V, 34.49y, a = 1.355". ADS 10157A*, 10.5y, a = 0.08". ADS 10157A is var. suspect NSV 7915. Secondary A5V, optical. ADS 10173AB, binary. E?, amp. 0.03V. Companion questioned. Alpha CV, 5.21 - 5.27V, amp. 0.04U, 1.31159d. V776 HerSecondary = GC 22634, 6.47V A8m. Primary, fast rotation, not Am. EB 6.1 - 7.00v, 0.6614261d. Period varies. Contact binary. Temperature discontinuity at interface. All photometric indices variable. Four-color measures by Gronbech and Olsen give +0.129(b-y), +0.184(m1), +0.887(c1), 2.810(beta) from 3 observations. V1010 OphLb 5.83 - 6.03V. V636 HerLong per? CPM with HR 6252 at 346". EB 2.80 - 3.08B, 1.44026907d. Semi-detached system. 6.51 - 6.61V, HeI, NII 4097 var. 3.5d. V919 Sco5.5 - 5.54V. CPM with 6247 at 346". BC 9.0, 9.1, 56.75y, a = 0.267". AxBC physical. ADS 10227A, Alpha CV 4.78 - 4.83V, 3.8567d. K line varies, 3.88d. V637 HerAmp. 0.14V. Component F, 7.3v O6, vsini 125k/s. 6.29 - 6.34V, 2.631? or 6.28 or 6.85d. V900 ScoAmp. 0.09V. Variations in HeI, NII, OII suggest turbulent outer layers. Innes and IDS data on components and number of components appear inconsistent. Probably different cluster components measured. AB, CPM. V823 Her3.6 - 3.64V. Companion F4p. Either runaway, or P Cyg type with extended expanding atmosphere. Amp. 0.07V. Amp. 0.04V. Time scale of 1d suspected. Third component 14v at 20". EB 6.07 - 6.69V, 7.84818d. V861 ScoDelta Sct 6.32 - 6.36V, 0.11505449d. V644 HerCPM. AC, CPM. C, 12.5v at 93". 6.7 A3V, 6.9 A4V, 37.9y, a = 0.181". Combined mag., colors. Lb? 3.14 - 3.20V, 4.1 - 5.0p. Possible nearby star on basis of spectroscopic parallax. Gamma Cas 6.11 - 6.20V, time scale 1d suspected. V828 AraSuspected occultation double. A8, F3, sep. 0.107". Delta Sct?, 4.85 - 4.91V. All companions optical. B is A8V, C is F5V. 7.1 F1V, 7.3, sep. 1.02", 577.85y, a = 1.183". EA 4.22 - 4.28V, 39.4809d. Fixed sep. ADS 10310A, Alpha CV 6.26 - 6.34V, 6.00925d. Spectrum, magnetic field, RV, same period. Rotation 6.0087d. V451 HerE amp. 0.35V, 34.8269:d. V923 ScoBinary. H alpha profile variable. Component B of system with HR 6341. B, 11.0v at 1.5" CPM. ADS 10323B, 10 - 11.3v? Amp. 0.03 or 0.04y. Cycle of 8d in 1984 consistent with var. in Ca II emission. V2213 OphOld disk population runaway star. Optical. CPM. 6.7 - 6.9p. Optical. 6.2 A1V, 8.2 F3V, 137y, a = 0.415". Optical. Binary with HR 6370, q.v., B* 3.2y, a = 0.026"; or 7.4y, a = 0.013", 0.2 solar mass. (Some uncertainty if unseen astrometric companion is A* or B*.) AB 6.2 A9III-IV, 6.2 A9III-IV, 8.159y, a = 0.116". Mean mass 2.7 solar. Alternate orbit, 16.08y, a = 0.167". Combined colors. Speckle interferometry indicates companion 1 mag. fainter than primary at 0.079". However, speckle observations 1986.46 (at 7000 Ang.) give sep. 0.15". AB 3.0 A2V, 3.5 A3V, 88y, a = 0.86". Combined mag., colors. SabikDelta Sct? The visual companion is optical. A companion at 0.168" has been discovered by speckle interferometry. Ellipsoidal binary, 6.118 - 6.195V, 80d orbital period. V829 AraDelta Sct 6.19 - 6.23V. Period analyses of new and existing data by Reed and Welch (1988, AJ, 95, 1510) favor fundamental period of 0.088d with overtones of 0.052, 0.130d, with the fundamental and second values as radial pulsations and the third as nonradial. V620 HerComponent B, 10.42V, +0.52(B-V); component C, 11.40V, +1.55(B-V). Amp. 0.15V. V915 ScoAldhibahEmission lines variable? H alpha width and profile vary. Sep. 0.108". Speckle observations 1986.45 give 0.14". AB, CPM. Binary with HR 6402, q.v. CPM with CoD-26d12036, 6.34v K5V at 700", same parallax. CPM. AB, 3600y, a = 4.68". Component B is HR 6407. Combined colors. Combined mag. 3.08V. Mass A, 14 solar. Other components faint, optical. Circumstellar lines around both A, B. ADS 10418A. Discovered by W. Herschel in 1795. SRc 3.0 - 4.0v. 6-yr. period superimposed by variations 50 - 155d. Surrounded by envelope of 2x10E+05 solar radii, expanding 10k/s, mass loss 3x10E-08 solar masses/y. RASALGETHIADS 10424B, dG4, optical. SarinSep. 0.121". B is dG0, optical. ADS 10428A, EA 5.84 - 6.56V, 1.67734617d. Period changes. i 86.57d. Components 5.3 and 4.6 Suns. U OphAB 5.53 G8V, 8.65 M0V, 693.24y, a = 10.415", or 2205y, a = 23.90". Various published orbits range from 242 to 2205y. Combined mag., colors. Companion is F2V. Amp. 0.04V on time scale 3 hrs. and 0.05 on time scale 1d suspected. Sep. 0.108". Binary with HR 6425. Binary with HR 6424. AB 6.1 K3V, 7.6 K5V, 42.177y, a = 1.734" or 42.09y, a = 1.82", combined mag., colors. Component C, 9.9v M2, 32" physical. D, 12.8v at 15". Amp. 0.04. Binary. Combined mag., colors, sep. 0.200". Binary. ADS 10449A, EA 4.69 - 5.37V, 2.0510270d. i 75.9d. Semi-detached system. Polarization measures indicate light from primary reflected on photosphere of secondary. u HerDelta Sct 6.50 - 6.52V, 0.1874472d, secondary 0.1449461d. V2112 OphAB binary; A3, A6. C, 11.7v at 12" CPM. CPM. SRd? 6.28 - 6.32V, about 170d. VW DraCompanion G5III, optical. Gamma Cas? 5.22 - 5.25V on time scale of fraction of a day. Lb? 4.9 - 5.1v, amp. 0.16p. V656 HerBeta C 3.25 - 3.31V, multi-periodic 0.140531 and others ranging from 0.0464 to 0.1399d. B not CPM; optical. Amp. 0.4V. Possibly CPM and same RV as HR 6462, 50'N. Component B, A7V; C is optical. Recognized as triple system by speckle interferometry: single star G5IV and close pair of which the brighter component is F7V eclipsing, sep. 0.045". E, amp. 0.085V, 2.2299d. Also long period var. outside eclipse, amp. 0.04V, 83.2d; probably the rotation period of the G5IV component. V819 HerAB binary. Combined mag., colors. Component C, 7.6v at 103". Delta Sct? Fixed sep. Companion A6V, optical. Binary with HR 6485, q.v. Another companion with sep. 0.29" seen on 1981.47 (McAlister and Hartkopf). Unresolved on 1985.25 (Bonneau et al.). B, 14.0v at 15"; C, 12.5 at 37". dF7, CPM, sep. 0.100". Measured sep. 0.069" on 1985.5 by speckle interferometry. F0V, CPM. Lb 5.98 - 6.21V. V640 HerCompanion K0III, optical. LesathCompanion K0IV, optical. 2.76 - 2.90V. ADS 10583B, 8.5 - 11.0v. 6.00 G8IV-V, 6.10 G8IV-V, 46.4y, a = 1.02". Combined mag., colors. V949 ScoSep. 0.098". Seen double 1911 and 1923, elongated 1918, single 1957 and 1959, and unresolved by speckle interferometry 1976. MaasymBeta C 1.59 - 1.65V, 0.2137015d, secondary 0.1068518d, beat period 10.1605d. Also possible 0.04V eclipse. X-ray flare observed in vicinity Lambda Sco on 1 June 1975. SHAULAComponent B, B9V; C, B8V. Central star of open cluster NGC 6383, probably older than the rest of the cluster core and might have initiated star formation in the core and beyond. Ell?, 5.68 - 5.71V. RastabanSRb 6.41 - 6.56V, about 12d. V642 HerAlpha CV, amp. 0.041V, 9.74073d. Variability and physical parameters discussed by North (1987, A&AS, 69, 371). V2125 OphComponent B, 7.81V, +0.30(B-V), +0.05(U-B), A8IV, vsini 129k/s. Fixed sep. from A. 1.90 - 1.94V? SargasBinary with HR 6555. ADS 10628B, I, 4.84 - 4.91V. Binary with HR 6554. ADS 10628A, I?, 4.83 - 4.95V. KumaA* 2.08 A5III, 8.5y, a = 0.065". Resolved by speckle interferometry. Delta Sct? RASALHAGUECompanion, 9.53V, +0.36(B-V), -0.02(U-B), F6IV-V, CPM. Measured sep. 0.140" on 1985.5 by speckle interferometry. Delta Sct? Visual companion optical. Delta Sct?, 3.52 - 3.54V. 7.3 F5, 7.6, 101.3y, a = 0.653". Combined mag., colors. Delta Sct? AB 5.34 G0V, 7.95 K3V, 76.00y, a = 1.52". Combined mag., colors. Third component 10v dM1 at 740" CPM. Component B, F4IV CPM. Lb 6.2 - 6.57V. V626 AraBeta C 2.39 - 2.42V, 0.1998303d, 0.205430, 7.3316, 0.189512 and 2.591d. Delta Sct 4.20 - 4.26V, 0.053d. Beta C?, amp. 0.01V. Component B, F4V CPM. Suspected occultation double. AB 5.58 F4V, 11.1, 122.68y, a = 1.004". Component C, 12.8v at 155" CPM. Sep. 0.02", but duplicity uncertain. Visual companion CPM. Sep. 0.111". Possibly close double. CebalraiDelta Sct? CPM with HR 6610. Combined colors. Mag. for blend 5.59V. CPM with HR 6609. Visual companion ADS 10749B, optical. EA 6.18 - 6.36V, 3.894977d. V624 Her7.1 B9, 7.3, 34.00y, a = 0.157". Combined mag., color. CDelta 4.24 - 4.84V, 7.01225d. X Sgr6.27 - 6.39V. Amp. 0.05V on time scale 3 hrs and 0.08 on time scale 1d suspected. V3894 SgrEA 5.66 - 6.18V, 3.169128d. V539 AraBC 10.3 dM4, 10.8, 43.20y, a = 1.360". This close pair forms a wider physical binary with component A. Component B, 9.70V, +0.75(B-V), +0.19(U-B), F5V, binary. Component C mag. diff 5.36v at 70" from A. V826 HerBinary. CPM with HR 6637, not shared with components C,D. DsibanCPM with HR 6636. Companion A0IV. Fixed sep. SX Ari, amp. 0.05V, 1.658d. Spectrum variable. V957 Sco6.9, 6.9v, 160.759y, a = 0.37". Binary. Delta Cep 5.87 - 6.46V, 17.12413d, period varies. Atypical light curve. Possibly SB. Y OphE? Amp. 0.26V. V906 ScoAmp. 0.04V. Possible periods 4.45597, 4.4588d (North 1984, A&AS, 55, 259). V951 ScoGamma Cas 6.65 - 6.94V, 86.7207d, similar to Pleione (HR 1180). Spectrum var. with possible periods 2.5552 and 0.78906d, correlated with RV. V744 HerAB binary. C, 13v at 28" and D, 10v at 95" both optical. Speckle interferometry sep. 0.102". ADS 10875. Not certain which component is the var. suspect. Rapid change in difference between components. AB CPM; C, 12v at 34" optical. Beta C 5.81 - 5.84V, 0.13989183d. Shortest period and lowest luminosity of type. Effective temperature varies by about 1000K. Ratio max. to min. radius 1.031. V2052 OphSRd 5.34 - 5.54V, 68:d. V441 HerGrumiumCompanion F0. Fixed with HR 6693. Possibly 5 yr. period in He 10830 emission. Sep. 0.107". Closed from 0.114" to 0.065" between 1981.5 and 1984.3 (McAlister and Hartkopf). However, speckle observations 1986.44 (Blazit et al. 1987, A&AS, 71, 57) yield 0.085". Possible nearby star on basis of spectroscopic parallax. SRb 5.85 - 6.73V, 7.7 - 8.3p, 120.5d. OP HerSuspected occultation double. Amp. 0.08V. He 10830 variable. ETAMINSRd? 4.38 - 4.48V, 29:d. However, more recent photoelectric observations cast doubt on variability. Alpha CV, amp. 0.008V, 0.719d (Manfroid and Mathys 1985, A&AS, 59, 429). Spectrum variable. V2126 OphGamma Cas 4.55 - 4.85V. Also rapid flares to amp. 1.8m possibly from later type companion. V2048 OphComponent B, 13.7v F? at 7", optical. AC fixed. C, 8.12V, -0.02(B-V), -0.57(U-B), B1V, vsini 130k/s. Alpha CV 6.44 - 6.52V, amp. 0.04U, 0.517468d. V771 HerBinary. ADS 10990B? 8.0 - 10.0v. Binary with 6729. AB 5.24 F2, 5.94 F3, 280.03y, a = 1.494". Component B is HR 6733. Color for combined light. Spectrum for combined light, F4IV. C, 11.28V, +0.78(B-V), +0.33(U-B) at 100", optical? AB CPM. C, 13v at 55" optical. 5.17 - 5.19B. Observations satisfy the SB period. V820 HerADS 11029A is speckle interferometric double, sep. 0.116". Visual companions, 13.5v at 33" and 13.5v at 48". ADS 11029A, CDelta 4.30 - 5.08V, 7.594710d. Period changes. Spectrum and magnetic field variable. One component of SB. Although HR 6742NashBeta C? 6.10 - 6.15V. Period varies from 0.284653 to 0.323d. V986 OphAB 5.7 A5V, 5.7 A5V, 191.23y, a = 1.063". Component B is HR 6750. Color for combined light. Combined mag. 4.95V. AB 4.20 K0V, 5.99 K4V, 88.13y, a = 4.545". B is 6.00V, +1.15(B-V), vsini =<25k/s. Aitken listed 9 additional faint companions within 180". Both companions optical. AB binary. B = HD 165474, 7.45V, +0.30(B-V), +0.17(U-B), A7pCrEu:Sr: or A8p (beta CrB), vsini 12k/s. ADS 11056B. Magnetic star; possible spectrum variable. Component B, B9V, optical? 5.1, 5.9, sep. 0.26", doubtful duplicity. Discordance in designations of components between ADS and IDS. We accept IDS. Component B, in notes to ADS 11076 not assigned letter: doubtful, sep. 0.1" if real. C, 14v at 25" CPM. D = ADS C, 11v at 54" optical. Visual companion is blue. EB 6.43 - 6.88V, 2.24815d. Mass transfer indicated. The var. is probably the 8.85V companion of the visual double. GCVS gives combined light. V3792 SgrAB 5.10 F7V, 8.50 K4V, 55.8y, a = 1.00". Optical. Gamma Cas 3.81 - 3.9B, 4.1 - 4.2p. Binary. Combined mag., colors. Component B is F0IV or F0V. Binary with HR 6782. Primary is speckle binary, sep. 0.106". Component C, 11v at 76". A companion to A at 0.106" discovered by speckle interferometry. Combined light of 6781-2 varies; uncertain which component the variable. Binary with HR 6781. Companion A6V, optical. YildunAB 6.07 F2V, 7.03, 270.0y, a = 1.16". Companion not confirmed. AB visual double, A4V, F0, combined mag., color. Third component found by lunar occultation, 1.3B, 0.9R fainter than B, sep. 0.024". Companion, 11.52V, +0.66(B-V), +0.11(U-B), F8V: Amp. 0.013v, 2.8855d. V4045 Sgr6.5 A, 7.2 F2, 3040y, a = 1.500". SX Ari, amp. 0.05V, 1.67d or 0.83d. V692 CrACPM. Binary with HR 6810. Binary with HR 6809. Faint component C at 221". ADS 11169A is SB, 4.1, 7.0v, sep. 0.011". Closest visual companion is B, 11.5v, B9III at 17"; C is 13.5v at 26"; D, 9.9v, B3; E, 9.4v, B2V, physical, vsini 184k/s. ADS 11169A, EA 3.79 - 3.92V, 180.45d. Also irregular changes in brightness. AB measured sep. 0.102" on 1985.5 by speckle interferometry. ADS 11149B, 8.5 - >11?v. Amp. 0.14B. V669 Her5.29 - 5.37V, correlated with H alpha emission. Companion A3V. Double may be spurious: companion not seen in 1934. Lb 3.08 - 3.12V. B, 9.68V at 39"; CD, 8.7, 10.2v, sep. 16.5". EA 6.0 - 6.9p, 2.4156832d. Period changes. Component A of visual double. RS SgrAmp. 0.10V. Companion A3V, optical? Three faint companions form compact group at about 95". Primary of visual double and a suspected astrometric binary. Optical. Kaus MeridionaliV4028 SgrCDelta 5.40 - 6.10V, 5.77335d. Y SgrADS 11271B, 12.08V, +1.08(B-V), +0.50(U-B). May have close fainter white dwarf companion. Amp. 0.01v, 6.3d. Weak variable magnetic field, 14.6d. V4050 Sgr6.11 - 6.14V. Emission variable 12 to over 22 yrs. KAUS AUSTRALISCompanion is A5:. 6.8 F6III, 7.0 A7IV, 240y, a = 0.59". Combined mag., colors. ADS 11320B, 12.9v at 17", CPM. ADS 11320A, I, 7.9 - 8.7p. AlathfarAB 6.5 A2V, 7.5 A4V, 775y, a = .90". Combined spectrum A5; component B, A8V:. Kaus BorealisOld disk population runaway star. 4.6 - 4.64V. AB physical. B is F5V, vsini =<54k/s. Component P, vsini 80:k/s. ADS 11353A, 4.9 - 5.9v. d Ser4.4, 6.1v, 271.7y, a = 0.392". Alpha CV, amp. 0.04V, 1.71646d. Same rotation period. AB binary with slow orbital motion. Combined mag., colors. B is A5p, vsini 80k/s. C, 7.1v F6V at 90" CPM. Some discordance whether B or C is the brighter. B, 12.6v at 6". Possibly CPM and common RV with HD 170051, 6.9v B5 at 185". Amp. 0.24V. A* 3.57 F7V, 0.768y, a = 0.124". Masses 1.5 and 1.1 Suns. Shortest known period for astrometric binary. Speckle interferometry indicates component A is binary, sep. about 0.1". B, 12v K1V at 149"; C, 13.5v at 10". Amp. 0.10V. Spectrum (Balmer emission lines) variable. V4031 SgrAmp. 0.012v, 2.21d. V432 SctAB, CPM. Primary is speckle binary, sep. 0.149". Component B, 11.8v, A7Vp; C, 12.8v, F5V, optical; D, 12.9v, F8V. A fifth companion at 0.149" from A discovered by speckle interferometry. Binary. CPM companion A0V. CDelta 6.34 - 7.08V, 6.744925d. May have blue companion. U SgrCPM with HR 6953. CPM with HR 6952. 0.945099d, amp. 0.03U. MV SerDelta Sct? Suspected binary probably single star. Companion optical. H-emission var. H-line widths vary in cycles of about 6 yrs. Amp. 0.10V. 6.3 G9III, 6.5 G7III, 210.9y, a = 0.416" or 190.8y, a = 0.418". Combined mag., colors. AB 6.8 G2V, 7.0 G2V, 292y, a = 1.358", or 3083y, a = 6.7811". AB 6.1 K0III, 6.1 G9III, 169.50y, a = 0.243" or 184.6y, a = 0.255". Component C, 8.8v at 26" physical. Hydrogen line widths vary in cycles of about 6 yrs. Amp. at 0.58 micrometers about 0.10m. Primary is speckle binary, sep. 0.141"; both ADS companions optical. Possible binary listed by D. W. Dunham, 6.5, 6.5, sep. 0.1". AB, fixed sep. Alpha CV?, 5.40 - 5.45V. AB 7.2 F9V, 7.3 F9V, sep. 0.13", 12.18y, a = 0.196". Measured sep. 0.141" on 1985.5 by speckle interferometry. Third component 14v, optical. Vega is the westernmost star of the Summer Triangle. It is the fifth brightest star in the sky and is approximately 25 [G/light year]s distant. It is over 2 1/2 times the diameter of the [G/Sun]. Companions in IDS optical. BD=+38d3231, 8.6v, 23' N. prec., may be CPM. Delta Sct -0.02 to +0.07V, 0.19d. VEGAAmp. 0.05V. Optical. Lc 5.80 - 6.35V, 7.3 - 7.8p. XY LyrCompanions probably optical. C at 108" may be brighter than B. Sep. 0.14" by Couteau; 0.175" by McAlister et al. from speckle interferometry. Component B, 10v, gK, optical. AC, CPM? A may be close binary, about 10d orbital period. ADS 11581A, Delta Sct 4.98 - 5.16B, 0.193770d, 0.11636d. Beat period 5.24774d. Other periods 0.095129, 0.186872, 0.838d. This "prototype" Delta Sct star is the least typical of its class. Component B, K0. Amp. 0.07V. Occultation double. SRb 6.05 - 6.58p, about 50d. V3879 SgrListed as double by Innes but probably not. AB fixed, B at 25", 8.05V, -0.05(B-V), -0.25(U-B), B8V, vsini 150k/s. AP, measured sep. 0.145 on 1985.5 by speckle interferometry. Duplicity questionable. 4.1, 4.1v, sep. 0.13", doubtful. Gamma Cas?, 5.00 - 5.05V. Amp. 0.15V. ADS 11640AB, >5600y. Both components close binaries. Speckle interferometry 1985.5 gives sep. Aa = 0.141"; Bb = 0.137". Alpha CV?, 5.04 - 5.05V. AB 5.00 A2n, 6.10 A4n, 1165.6y, a = 2.78". Binary with HR 7052 = B, and CPM with HR 7053-4 at 208". Combined mag. and colors for HR 7051-2 are 6.48V, +0.19(B-V), +0.04(U-B). See HR 7053. Fixed sep. ADS 11670A, I, 5.64 - 5.81V. CPM with HR 7057 = ADS 11639D. Other components optical. Delta Sct? CPM with HR 7056. Alpha CV 6.41 - 6.58V, 10.1353d or 9.975d; also spectrum, magnetic field, RV. V535 HerAB binary, B, Am, F3Vm, or Am(A5/F1/F2), RV +9.2k/s, vsini =<25k/s. C, 11.3v optical. All companions probably optical. Discovered by Pigott in 1795. RVa 4.45 - 8.20V, 140.05d, period varies. Variable He 10830 and Ti emission. Largest intrinsic polarization in UV at minimum light. Light and RV periods differ. R SctGamma Cas 3.4 - 4.3V. Suspected occultation double. 6.69 - 6.82V. Possible nearby star on basis of spectroscopic parallax. B, 12.5v at 23"; C, 8.14V, +1.05(B-V), +0.75(U-B), K0II-III. delta, epsilon in cycles of 3 yrs. Gamma Cas 5.68 - 5.99V, 6.696d; also about 2400d with amp. 0.2m. H alpha profile varies in period about 7d; H gamma, CX DraADS 11726A, SR 9.7 - >10.9p, 148.0d. S SctBinary, companion K3III-IV. B, 10.89V, +1.05(B-V), +0.76(U-B), at 35"; C is G0V. 5.98 - 5.98V. Cycles 7.5d? AB fixed. B is 8.6v, B7v; may be collapsed star; vsini 120k/s. E, 9.9v A8pSr or B9V at 67" optical? F, 9.9v A8-9V or or B9V at 86". A, B, E and F are CPM. ADS 11745A, EB 3.25 - 4.36V, 12.913834d. Period varies. Presumed disk around secondary. Also radio flare activity. Prototype Beta Lyrae type, discovered by Goodricke in 1874. SheliakCW 3.94 - 4.75V, 9.088d. Period changes. EB 6.12 - 6.30V. V822 HerAB fixed, combined mag., colors. C, 11.21V, +1.25(B-V), +1.20(U-B), at 28". Ain al RamiInterferometer measures indicate multiple star. NUNKIB is K3IIIp optical, vsini =<54k/s. C, 11.5v at 139" is receding from A. Alpha CV 5.25 - 5.41V, 3.6733d. Similar period for He-line intensities, magnetic field. V686 CrAC, 11v at 38" optical. SRc? 4.22 - 4.33V. Del2 LyrABC fixed. B, 10.2v at 2". C, 7.69V, -0.08(B-V), -0.28(U-B), variously classified B8V, B9.5IV, A2, F3. Binary with HR 7142. 4.59 - 4.72V. AlyaBinary with HR 7141. V828 HerHigh-velocity star. EW 4.74 - 5.00V, 0.5914264d. AB observed as single round image in 1974. Suspected occultation double, equal components. SRb 3.88 - 5.0V, 46.0d. R LyrHydrogen line widths vary in cycles of about 10 yrs. 6.6 F8V, 6.6 G0, 13.58y, a = 0.131". AB 5.36 G0V, 7.46 K1V, 61.203y, a = 1.24". Combined mag., color. Components C, D, optical. Suspected occultation double. Companion blue star? ADS 11884A, CDelta 5.18 - 5.68V, 4.470916d. Magnetic field. Possible blue companion. FF AqlBinary. B1, B9. Amp. 0.053B. Alpha CV 5.83 - 5.93V. Published periods of 6.05 and 9.78d probably spurious; nor does a more recent 6.5386d satisfy all observations. Period may be years. Abt and Golson found range 5.83 - 5.91V. Two isolated obs. of 5.93 and 5.94V, while other observers report intermediate values with amp. <0.015V. V1286 AqlCPM with HR 7170. Combined mag. 5.82V, -0.03(B-V). CPM with HR 7169. Both companions optical. Deneb el OkabB, 12.1v at 13", optical. SulafatCompanion 9.80V, +0.21(B-V), +0.07(U-B), A5V fixed. 6.9 A1V, 7.2 A3V, 259.07y, a = 0.601". Combined mag. AB CPM. B is G8V. AB 3.2 A2III, 3.4 A2V, 21.138y, a = 0.532". AscellaSuspected occultation double with equal components; combined mag., color. vsini of secondary 150k/s. AB CPM. B, 9.17V, +0.47(B-V), +0.09(U-B). Probable double, 7.1, 7.1v, sep. 0.05". Sep. 0.099". Consistently unresolved by speckle observations at five epochs between 1977.48 and 1981.47 (McAlister and Hartkopf). B, 10v at 44" optical. SRb 6.6 - 8.4v, 10.6 - >12.4p, 353d. Mean mag. varies in cycle of about 2270d. V AqlDelta Sct 6.58 - 6.62V. Period analyses of new and existing data by Reed and Welch (1988, AJ, 95, 1510) imply radial pulsations of 0.099d and 0.060d with no evidence of nonradial pulsations. LT VulEE DraCompanion gK4, optical. See HR 7226. Delta Sct, amp. 0.05V, 0.04B, 0.097d. Polaris AustraliAxBC binary, BC 9.2, 9.8, 138y, a = 0.195". Variable on short time scale with uncertain 0.33772d period. Manfroid and Mathys (1985, A&AS, 59, 429) also give possible 0.48773d period. Magnetic field not detected (Borra and Landstreet 1980, ApJS, 42, 421). Deneb el OkabCompanion A0V. E 5.02 - 5.06B, 1.30227d. Form of light curve possibly variable. Y AqlAmp. 0.2V. V4024 SgrAlfecca MeridianAB binary. Other companions probably optical. Resolved by speckle interferometry 1986.45, sep. 0.08". AB, combined mag., colors, sep. 0.093". Third component 6.0v at 0.4". Albaldah7.0 K3III, 7.2 K2III. Unresolved by speckle interferometry. Probably not double. AB binary, B is G5. Speckle interferometry indicates a fourth companion at 0.089" from A. Amp. 0.05V. V1762 Cyg6.1 A2N, 6.5, 157y, a = 0.56". Alpha CV 5.91 - 5.98V, amp. 0.03U, 0.03c1, 0.05m1, H-beta 0.015, 1.160898d. V471 LyrB, 8.0v at 0.7" CPM. C is G5. Companion optical. Alpha CV 5.06 - 5.16V, 1.73d. V1288 Aql5.5 F8V, 5.7 F9V, 18.75y, a = 0.153". Component A is SB, 6.2, 6.2v, sep. 0.001". Binary with HR 7294. C, 12.7v at 56" optical. Possibly high luminosity evolved helium star. RCB 6.0 - >15.0v. Also pulsations 38.454d, changing amplitude. Observations 1984-86 indicate semiregular pulsations of 33 to 40d, 6.13 - 6.78V, 0.38 - 0.76(B-V), -0.09 to +0.52(U-B). RY SgrB is A0, optical. AladfarBinary. Companion A1V. Suspected occultation double. AB binary. C, 10.1v at 48" from A; D at 50", mag. diff 5.54V. AB CPM, B is 9.07V, +0.14(B-V), -0.05(U-B), F8V or G0IV, optical? Speckle interferometry indicates a fourth companion at 0.051" from A. Delta Cep 5.99 - 6.35, 1.49078 or 1.49107d. Period variable. Also 1178.5 and 2655d. Amp. variable in 1063.5d. If Pop. I, shortest known classical Cepheid in Galaxy. V473 LyrNodus SecundusAB, CPM. AB binary. ADS 12287A, Beta C? 5.4 - 5.46v, 0.6096d. ES VulAB binary. C, 13.7v at 12" optical. EA 6.58 - 9.18V, 3.3806260d. Period varies irregularly. i 90d. Semi-detached system. U SgeNearby star suspected of variability from photometric discordances by different observers. Delta Sct 5.51 - 5.57V. Period analyses of new and existing data by Reed and Welch (1988, AJ, 95, 1510) indicate a possible change in pulsational modes during the last several years, with fundamental period of 0.146d and possible nonradial pulsations of 0.141, 0.183, and 0.091d. V1208 AqlB probably optical. Possible X-ray source 3U1915-05. Old disk population runaway star. CPM. Companion A5V; vsini 129k/s, optical? Arkab PriorComponent B, K2IV, RV -3; component C, G5:III, optical. Sep. 0.036". Questionable occultation double. Delta Sct 3.90 - 3.93V, 0.050d. Spectrum var. 8.115813d. EB 4.34 - 4.44p, 137.939d. Irregularities in light variation. Variable polarization, probably due to circumstellar dust. Arkab PosteriorRukbatOptical. 5.8 A8, 5.8 A6-F0, 10.8y, a = 0.123". Probable occultation double. Speckle interferometry 1985.5 gives sep. 0.081". Chi1 Fl 47AB, CPM. Unresolved by speckle interferometry 1986.46. Component A astrometric binary, A* 3.36 F0IV, 3.422y, a = 0.058"; unresolved by speckle interferometry. Delta Sct? Proper motion slightly variable? H alpha emission variable. Both companions optical. Components B-D are 40" to 90" from A. A new component at 0.181" found by speckle interferometry. Colors of B are +0.31(B-V), +0.16(U-B). Components B, 10.8v at 27"; C, 10.46V, +0.61(B-V), +0.08(U-B), at 73" and P, 14.5v at 26" all optical. Alpha CV, amp. 0.02U, 0.68674d. V1741 CygBinary. B, 8.69V, +0.86(B-V), +0.32(U-B), G1IV-V. AB fixed. C, 7v at 2", binary. ADS 12503A, CDelta 6.08 - 6.86V, 7.02393d. Period changes. U AqlSecondary K0. Anser (rarely usAmp. 0.1B. B, optical. Gamma Cas, amp. 0.12V, 0.8518d. Variation may be due to rotation and inhomogeneous distribution of brightness on disk. V923 AqlAmp. 0.015v, 2.92133d. PW TelLocated at the head of [X/Cygnus] the swan, Albireo is a unique binary star system that lies about 190 [G/light year]s away. One star in this system is a yellow star while the second star is a hotter, blue type star. 7270.2y, a = 62.90". Binary with HR 7418. vsini of B-type component of ADS 12540A 50:k/s. Component C, 11v at 50". Two additional components of A resolved by speckle interferometry: Aa 1981.70, sep. 0.42"; Ap 1978.41, sep. 0.12" and 1979.46, sep. <0.08". ALBIREOSee HR 7417. Unresolved by speckle interferometry 1981.47, sep. <0.03". E, amp. 0.13V, 4.62988d. V4089 SgrRS CVn. Amp. about 0.045V, 108.5707d. Variable H alpha emission. V1817 CygB and C optical. Primary of SB Delta Sct? Amp. 0.015V in about 10d. CPM. ADS 12654. Uncertain which component varies. Visual companion CPM. SRb?, amp. 0.18V, 40:d. V1743 CygFixed. Companion K0III. CDelta 6.78 - 7.51V, 7.990676d. U VulDelta Sct oscillations with periods 94.1 and 115.7 min. QQ TelAlsafiB is B8, optical. V4090 SgrAP, sep. 0.1" unresolved by speckle interferometry at eight epochs between 1976.45 and 1981.70 (McAlister and Hartkopf). AB CPM. B, 13v at 3". C, optical. Sep. 0.200". B, 12v K0Ve at 48" optical. C, 12v at 130". Rotational velocity of A 123k/s, of B 142k/s. ADS 12737A, EB 5.18 - 5.36B, 1.95026827d. i 71.7d. Spectra vary in period 1.950271d. CPM companion B3V. Primary is close double, combined colors. Mag. for blend 5.30V. Component B, 12.6v at 38" optical. C, 8.9 F8V at 46" physical. Amp. 0.09V. 1.188y, a = 0.026". Companions B and C optical. ShamA companion at 0.084" discovered by speckle interferometry. AB binary. EA 5.85 - 6.37V, 7.6407613d. V1143 CygCompanions probably optical. Speckle interferometry 1985.5 gives sep. 0.178". Primary of visual double, EA 5.93 - 6.05V, 2.513294d. Double unresolved in 1961 when period changed sharply. QS AqlSuspected visual double, but may be single. AB, fixed sep. Delta Sct 6.50 - 6.53V, 0.088d. V1276 CygBinary with HR 7504. Third component mag. diff 7.17V, sep. 70" from A. See HR 7503. E? Amp. 0.076V. PS VulLb 6.33 - 6.55V. B-V from +1.57 to 1.62. V1351 CygCDelta 6.44 - 7.22V, 3.8455473d. Period changes. SU CygHigh space velocity. SRb 7.8 - 8.6p, about 40d. V973 CygDelta Sct 6.04 - 6.06V, 0.080d. NZ PavTARAZEDAB 2.91 B9.5III, 6.33 F1V, 827.6y, a = 3.20". ADS 12880A is NSV 12381, 2.85 - 2.89V. Component B is NSV 12380, 6.5 ->8.5v. AB binary. B is 7.16V, +0.02(B-V), -0.07(U-B), B9.5V, vsini 250k/s. Component B, 8.56V, +0.05(B-V), +0.11(U-B), A2V at 39". AB binary. B is dK6. Component C, optical. ADS 12913AB and ADS 12889 (9.2, 9.4 dK5 sep. 3") at 792" are CPM and have same RV and parallax. ADS 12889, 259y, a = 2.27", mean mass 0.6 solar. ADS 12913B, 8.55 - 8.60V; difference between components varies from 1.9 to 3.3p. B, 13v at 3" binary with A. C, 14v at 10" binary with A. D, optical. Suspected visual double probably single image, composite spectrum. Secondary either B6 or A0V. Amp. 0.09p. Amp. 0.12V. 6.1, 11.9v sep. 2" in 1910, 1913, not seen as double in 1926, 1928, 1929. Probably single? AB, >3000y. AB 5.5 A1V, 6.2 A3V, 22.8y, a = 0.146". Masses 4.0, 2.0 solar. C, 8.7v at 8" physical. Speckle interferometry 1985.5 gives sep. 0.180". CPM with HR 7549. CPM with HR 7548. 7.2 F5V, 7.7 F7V, 156.52y, a = 0.624" or 157.21y, a = 0.607". Combined mag., colors. 6.44 - 6.50V. V1765 Cyg5.28 - 5.33V, 2445.2d. Revised period 2300d. Variable magnetic field and spectrum. V3961 SgrOptical. Gamma Cas? 6.33 - 6.52V. V1339 AqlAltair is the southernmost star of the Summer Triangle. The 12th brightest star in the sky, Altair is only 16 [G/light year]s from us. This star rotates extremely fast, once every 6 1/2 hours. For comparison, our [G/Sun] rotates once every 25-30 days. Component B optical. ALTAIRComponent B optical. AC, 13.8 dM4, 22" binary. Delta Sct 6.29 - 6.35V, 0.100d. CN DraDiscovered by Kirch in 1686. M 3.3 - 14.2v. Period changes: 1686-1842, 405.88d; subsequently 408.05d. Variable CO emission from circumstellar envelope and enhancement of shell at minimum light. Total visual absorption of shell = 2 mag. Variable SiO maser source. Appreciable reddening at ascending light. Amp. at 0.58 micrometers about 0.11m. H line widths vary in cycle about 15 yrs. Component B, optical. Lb 5.08 - 5.4v. V1509 CygEA 5.61 - 5.78V, 12.42612d. Period changes. V380 CygDiscovered by Pigott in 1784. CDelta 3.50 - 4.30V, 7.176641d. Period changes. Variable He 10830 in emission and absorption. Speckle interferometry indicates companion at 0.291", probably not the same as the SB or occultation binary. EA 6.48 - 7.51V, 1.18287511d. Period decreases about 0.49s/y. i 80.3d. Contact binary. Masses 2.2 and 1.2 solar, radii both about 2.2. V505 SgrComponent B = A3V. E?, 6.20 - 6.25V, amp. 0.06B, over 80d? Variable polarization. Expanding atmosphere. Alpha CV 5.61 - 5.67V, 224.5d. Also period for spectrum and magnetic field var. Rotation 226d. V1291 AqlI 6.4 - 6.52p. Variability suspected on basis of comparison stars, both of which are either variable or suspected of variability. Optical. BY Dra type predicted, but variability not yet detected. Binary, companion K5III (AJ, 82, 431, 1977). However, Buscombe points out that the companion is F6V and this is more consistent with the magnitude difference between the components, if physical. TylAmp. 0.05B. CPM with HR 7594. CPM with HR 7593. TerebellumOptical. Speckle interferometry 1985.5 gives sep. 0.173". Old disk population runaway star. Beta C? 6.26 - 6.30V, 0.3775d. V819 CygAB binary. B 12v dM3 at 13". ADS 13110A, amp. 0.05V. ALSHAINTerebellumCDelta 5.28 - 6.04V, 8.382173d. Period varies. Spectrum varies, F6Ib-G5Ib. S SgeAB CPM. B, 12v at 7". Other components optical. AB combined mag., colors. Sources differ on spectral class of component B from A7V to F4V. vsini of B, 120k/s. SRb 4.91 - 5.26V, about 80d. NU PavAmp. 0.07V. AB and AC binary. C, 9.0v Am(A2/A8/A8) at 3", physical. Lb? 5.27 - 5.57V, 7.0 - 7.24p. VZ SgeGamma Cas + Beta Cep, amp. 0.07V, 0.20:d. V1746 CygL? 4.45 - 4.61V. V3872 SgrAmp. 0.03V, 14.0d. NT VulSuspected occultation double. 3.52 - 3.65V. Companion 16.4pgM6, CPM. Discovered as double by W. Herschel; companion not rediscovered. SRd 6.18 - 6.55V, 28.49d. V1401 AqlLb?, 4.89 - 4.94V. Optical companion, +0.74(B-V), +0.34(U-B). Amp. 0.08B, about 26d. Mass loss 0.00005 solar masses/y. V1768 CygCPM. B, 13.2v at 12", optical. C, 12.5v at 40". AD CPM. B, 13.7v at 23"; C, 11.6v at 36". 5.36 - 5.41V. Binary. AB CPM. B, 11v dM5, sep. 6.6". Wroclaw contr. no. 16 gives mag. differences but no sep. for four components: AB 5.4v, AC 5.15, and AD 4.0. Possible misidentification? Discovered by John Herschel as simply double. Components C and D apparently first listed by van Albada at Lembang in 1958; only magnitudes and no separations were indicated. Precedes HR 7703: error in HR catalogue. AB binary. B, 8.7v at 13". C, optical. SX Ari 4.91 - 4.97V, 0.07d. Possibly also Gamma Cas type. H-line widths vary in cycles about 15 yrs. V1624 CygAmp. 0.3V, 0.09U, 16.82d. Magnetic var. Discordance as to which component has the peculiar spectrum usually attributed to A. However, on the basis of better spectrograms, Abt gives A = A0V, B = A0Vp(Sr,Cr st.,Ca wk.). S, 5.87 - 5.92V. Binary. AB CPM. Component D of ADS 13554 of which primary is HR 7735. Delta Sct? There is very muDelta Sct, 16.478d, amp. 0.07V. NU VulComponent C, 6.99V, -0.14(B-V), -0.58(U-B) B5V, vsini : 25k/s, at 107" fixed. AP probably single star. ADS 13554A, EA 3.77 - 3.88V, 3784.3d. Amp. varies strongly with wavelength. C = NSV 12931, 6.98V. B is K1III, optical, vsini =<54k/s. Delta Sct 4.94 - 4.97V, 0.031d. Lambda Boo-type star in Delta Sct instability strip. V1644 CygAB and AC both binary. C, 9v at 12". AB CPM, 680?y. 4.60 - 4.80V. Sudden brightening in 1982, amp. 0.18V. QR VulDelta Sct? E, amp. 0.367U, 0.142B, 0.052V, 0.031R, 0.010I, 249.099d; duration of primary eclipse <17d. QS VulCPM. See note for HR 7754. ADS 13632B, 14v at 44"; C, 9.6v K5III, at 45" physical, vsini =<54k/s. D, 14.3v at 29" from C. Prima GiediEA 3.90 - 4.14V, 1147.4d. Period varies. Light var. outside eclipse. The K component may be slightly intrinsically variable. V1488 CygIDS notes Alpha1 Cap = HR 7747 (ADS 13632, four components) as one of five components of Alpha2 Cap = HR 7754 = ADS 13645. Hence, we have recorded n = 9 for both. ADS 13645AB optical; BC 11.2, 11.5v, sep. 1.2" binary. Secunda GiediPossible radio source. SD 3 - 6v. Since 18th century, 4.6 - 5.6v. Shell star, Nova 1600. P CygComponent C, photometric spectral class A2IV, vsini 53k/s. Component B, 10.1V at 4.1". For component AB, Rakos and Mermilliod give 6.93V, +0.28(B-V), +0.24(U-B). However, other sources give the following V magnitudes: Comp. 1976 1978 1980 Preferred Gronbech and Oblak Ruffener Olsen AB 6.635 6.610 6.608 6.61 C 7.724 7.706 7.72 Colors converted from the uvby system (Gronbech and Olsen) are AB +0.13(B-V), +0.185(U-B); C +0.165(B-V), +0.14(U-B). AB binary. C, at 34", 11.11V, +0.19(B-V), -0.29(U-B), B7Vp:, vsini 340k/s. D at about 45", 11.17V, +0.19(B-V), -0.32(U-B), B8Vp:, physical, vsini 279k/s. Primary is speckle binary, sep. 0.047". Amp. 0.06V. CPM. AlshatDelta Sct? Complex system with HR 7776, CPM at 205". ADS 13717A is occultation double, 6.2 - 8.3v, sep. 0.8"; also 7.2, 7.2v, sep. 0.05". Component B, 10.2v, A1, binary with A at 0.9". A is astrometric binary. The close occultation pair is questioned; it has not been confirmed by speckle interferometry. Complex system with HR 7775, q.v. Component B, vsini 97k/s. Occultations indicate component A is multiple system: 4.0, 4.3v sep. 0.0002", 4.8v at 0.022" and 6.7v at 0.0001". A also suspected astrometric binary, 3.07 F8V. Possibly also two faint 13v components at 112" discovered by John Herschel. DabihAmp. 0.05V. Variability agrees with spectroscopic period. V1773 CygAB binary. B is dF3. AB 6.33 A2V, 8.87 F6V, 69.86y, a = 0.2766" or 90y, a = 0.214". Component C, 9.2v at 3" also binary with AB. Alpha CV, amp. 0.04V, 8.5304d. Variable spectrum 1.132854d. V1584 CygAB binary. Combined mag., colors. BC, 9.2, 10.2v sep. 17.6". PeacockADS 12214, 18.75y, a = 0.153". EA amp. 0.15V, 5.298036d. DE DraNo physical relation between the radio components and the star. No demonstrable connection between Gamma Cyg and the so-called Gamma Cygni supernova remnant. SadrAB binary. B, 11v at 1.3". C and D optical. ADS 13786B, 8.5 - 11.0V. Discordances as to which component is B, which C. IDS gives B, 13.1v at 17.1". Lb, amp. 0.25B. AC DraCPM. 6.6 K2IV-V, 7.8 K1V, 232.76y, a = 1.225". Amp. 0.04V, pulsating. AB CPM. Probable spectrum variable. 7.1 A3V, 7.4 A5V, 83.72y, a = 0.172". AB binary. B, 8.0v at 0.8". CPM. Secondary, A2V, vsini 75k/s. Omega CygCPM with HR 7830. CPM with HR 7829. AB binary. Also observed as occultation double, 6.6, 7.4v, sep. 0.1". BC 7.5, 7.6v, Am, measured sep. 0.108" on 1985.5 by speckle interferometry, vsini 63k/s. A, optical, with companion, measured sep. 1985.5 Aa = 0.341" by speckle interferometry. B component 8.5v, frequently invisible. Component B, 12.9v A5V at 18", optical. AB, CPM. B, 11.3v at 3". Binary. B is A2. Deneb DulfimDelta Sct amp. 0.03V, 0.11d. CPM. Companion G5V. AB sep. 0.1", no magnitudes cited. Both 2 micron IR and UV sources. Alpha CV 5.16 - 5.22V, 20.2728d. Also period of spectral changes and magnetic field. Var. in K-line profile suggests star spot rotation. Rotation period 20.2754d. AF DraAB 4.0 F5IV, 4.9 F5IV, 26.65y, a = 0.475" or 26.60y, a = 0.480". Speckle interferometry gives sep. 0.58" and with SB data leads to masses 2.2 and 1.8 solar. Combined mag., colors. Components C-E optical. RotanevOptical. Double with HR 7887 at 181". Third component 12.9v at 71". High space velocity. SRb 5.79 - 6.9v, 59.7d. Amp. 0.36V, 0.12(B-V), 0.19(U-B), but varies. EU DelDouble with HR 7885. AB 5.8 B6III, 6.3 B6IV, 200y, a = 0.31". Visual third component 13v at 159". Occultation fourth companion, 9.3V, sep. 0.052". Tau1 Fl 13 and TH alpha varies. AB optical. B, 11.8v at 29". AC CPM, C is K2IV. Both companions optical. AB optical. B, 13v at 7". Companions optical. SualocinB is BD+80d662, 8.71V, +0.63(B-V), +0.00(U-B), F8V, CPM. AB binary. C, 8.5v A0 at 69" CPM. Delta Sct? Binary. AB binary. Deneb is the easternmost star in the Summer Triangle. It is a blue/white supergiant star that is 60,000 times more [G/luminous] than our [G/Sun], although it is only 25 times more massive. It lies 1,600 [G/light year]s away. Alpha Cyg 1.21 - 1.29V. Change in H:H epsilon. No emission recorded before 1944. DENEBGamma Cas 6.40 - 6.68V. V568 CygDelta Sct 4.39 - 4.49V, 0.135547 and 0.154991d. Combined magnitude of two components. AB fixed. CDelta 5.85 - 6.91, 16.386332d. Period changes. X CygSRb 7.6 - 8.9p, 110d or 160 - 180d. Mean mag. varies in period 1100d. Amp. 0.26V, 0.04(B-V), 0.19(U-B). U Del3249y, a = 13.813". Binary with HR 7948. See HR 7947. AB optical. C, 13v at 78" CPM. Gienah CygniAlbaliLb 4.41 - 4.45V. EN AqrADS 14293. Uncertain which component varies. B-A changes by up to 3v. B is BD+57d2241, optical. Labelled UpsilonAB CPM. B, 10.03V, +1.27(B-V), +0.66(U-B). C, 13v at 14" optical. ADS 14290A, Lb? 4.91 - 4.96V. T CygSee HR 7959. AB 4.85 B5V, 6.07 B7V, 391.30y, a = 0.777". Combined colors. Mag. of blend 4.52V. Component C, 9v K2III-IV at 84", optical; vsini =<54k/s. Resolved by speckle interferometry 1986.45, sep. 0.87". Companion optical. Optical. Alpha Cyg 4.81 - 4.87V, no clear periodicity. Small variations in polarization have been observed, 2.0 to 2.6%. V1661 CygB8V+A3V. CPM. AB 6.4 F5V, 7.22 F8V, 187y, a = 0.855". Mag., colors for combined light. Old disk population runaway star. In Schurig's Atlas this is mistakenly labelled 58 Cyg for 56 Cyg. CDelta 5.44 - 6.06V, 4.435572d. T VulCPM. G8III-IV + G2.5IV. Delta Sct 6.55 - 6.58V, 0.054d. Per. and amp. may vary. EM AqrBeta C 6.2 - 6.43p, 0.20104071d. Sudden period change in 1972. 1924-70 per. increased 0.037s/y. BW VulFixed sep. Binary. Optical. AB fixed sep. B, 11.8v at 36". AB, CPM. H alpha profile variable. Possibly binary star. EB 5.95 - 6.25V, 1.575531d. Also Delta Sct amp. 0.1V, 0.12d. DV AqrBinary. Alpha CV, amp. 0.050V, 2.25d. AO CapAB 6.0 F5IV, 6.3 F7IV, 101.485y, a = 0.647". Combined mag., colors. Component C, 7.2v G0V at 11", CPM. 6.3 A5V, 7.6 F4V, 52.5y, a = 0.27". AB binary. CPM? Companion K0IV. AB CPM. B, 9.38V, +0.22(B-V), +0.04(U-B) A8III, vsini 97k/s. Component C, 12v at 26" optical. ADS 14526A, Gamma Cas 4.49 - 4.88V. Expanding circumstellar shell. Marked evidence of mass loss. Shell spectrum faded between 1973 and 1975. Metallic absorption lines disappeared. V832 CygSep. 0.110". 5.34 - 5.48V, probably eclipsing; same period as SB. V1931 CygAB 6.74 F5, 7.21, 3055y, a = 3.740". CPM with HR 8059. Duplicity of AB uncertain; sep. 0.110"? AB, combined mag., colors. CE optical. AB CPM. 9.1v A2 companion. CDelta 5.57 - 5.96V, 2.499215d. Period varies. DT CygAB 5.22 K5V, 6.04 K7V, 722y, a = 24.65". B is HR 8086. Aa x P, 4.9y, a = 0.014". Astrometric measures indicate 3 invisible companions, periods 6, 7 and 12y. Unresolved by speckle interferometry. Suspected planetary companion not substantiated. Proper motions for HR 8085 and 8086 taken from Luyten LHS. SAO has only one entry (component A?), but appears to give the mean position of A and B. 5.19 - 5.27V, 350 - 400d. V1803 CygSee HR 8085. ADS 14636B, Is, 6.02 - 6.09V. AB binary. B, 7.8v A0V or Am(A2.5/A7V/A9), vsini 80k/s. C, 9.2v K1III at 58" optical, vsini =<54k/s. ADS 14682A, 5.55 - 5.71V. Alternating periods of 1.12912 and 1.19328d. V 389 Cyg may be triple star, with long period about 150d, perhaps 110 or 270d. V389 CygAB binary, B, 11.6v at 2". C, 12.6v at 48" optical. ADS 14702A, Alpha CV 4.58 - 4.77V, 314d, 0 00868d. Magnetic field var. 1786d and 72y. Spectrum var. 72y. Fixed. Companion A4V. Delta Sct 6.41 - 6.48V, 0.097d. EW AqrCompanion B8V. AB fixed. B, 9.6v at 1.2". C, 7.29V, +1.55(B-V), +1.38(U-B), M5III, vsini =<25k/s. 6.5 A7V, 6.5 A7V, 17y, a = 0.11". Combined mag., color. White dwarf companion. 7.0 A7V, 7.0 A7V, 34.44y, a = 0.227". Combined mag., colors. Measured sep. 0.090" on 1985.5 by speckle interferometry. AB binary. B, 7v at 1". Amp. 0.045V. AB 5.2 F7V, 5.3 F7V, 5.70y, a = 0.26". Combined mag., colors. Component C, 9.5v at 48" optical. 6.44 - 6.50V. AB 3.82 F0IV, 6.42 G1V, 49.80y, a = 0.85". Components C, 13v at 29" and P, 12v at 72", both optical. Q, 12v at 90", physical. R, 13v at 90", CPM. Delta Sct 3.65 - 3.84V. 2-3 hrs.? Possibly variable period. Sep. 0.08". May be only single star. Kitalpha7.0 G2IV, 7.2 G2IV, 84.4y, a = 0.61". Combined mag., colors. Companion A7V or G0V. Old disk population runaway star. H alpha profile varies. SRb 7.7 - 9.4p, 320d. T IndAB CPM; 79000?y. Component B, 10.0v G8.5V, probably optical. 4.28 - 4.50V. AB binary. B is K4. Components D and E, 12v at 247" and 149" probably optical. Alpha CV 4.77 - 4.87V, 2.1215d. AB fixed. Ell?, 6.40 - 6.44V, 5.4d? 5.05 - 5.075V, 3.390d. V1809 CygSRb 8.6 - 10.3p, 233.3d. Y PavBinary, sep. 0.130", about 30y. Unresolved by speckle interferometry. Delta Cep 5.77 - 5.96V, 3.332816d. Uncertain which component of ADS 14859 is var. Perhaps Delta Sct type. V1334 CygADS 14858A, Delta Sct?, 2.41 - 2.47V. ALDERAMINAB binary. B is B3V. Variable shell spectrum. AB binary. Component B, G5IV. AB CPM. Companion K0V. Companions optical. Component B of which primary is HR 8193. Component A in system of which B is HR 8189. Other components 11.6, 13.4, 14.6v. ADS 14943A. All companions 10.5m or fainter. SRb 5.43 - 5.97V, about 50d. SX PavDelta Sct? V1934 CygADS 14969A. Companions optical. B 12.06V, +1.13(B-V), 33". C 10.38V, +0.46(B-V), -0.04(U-B), F5V, 54", vsini =<54k/s. Components B and C sometimes interchanged. Delta Sct amp. 0.01V, 0.044d. IK PegAlpha CV?, 5.20 - 5.30V, 0.726d. Amp. 0.06V. Optical. Both companions optical. SadalsuudADS 15032AB, 50y. B, 7.84V, +0.18(B-V), +0.06(U-B), A2.5V, vsini 60:k/s. Third component discovered by speckle interferometry, mag. diff about 4v. Sep. 0.025". Possible circumstellar material. ADS 15032A, Beta C 3.16 - 3.27V, 0.1904881d, modulation period 10.893d. SiIV and CIV vary. Satellite UV obs. indicate temp. varies 1340d, max./min. radius 1.038. AlfirkA* 3.76 K0III, 2.84y, a = 0.052". 6.7 A2V, 7.0 A4V, 173.9y, a = 0.293". Combined mag. A third component is suspected. Component A is SB, 5.0, 6.3v, 0.0047"; component B, 9.5v K1III-IV: at 68", physical, vsini =<54k/s. Gamma Cas 4.44 - 4.72V. Polarization variable. Slight variation in H alpha line width. SRb 6.8 - 8.9p, 131.1d; secondary period 235.3d. W CygCPM. Speckle interferometry indicates mag. diff 3.0, sep. 0.033"; D. W. Dunham gives 5.1, 7.1v, 0.07". AB CPM. B is 7.65V, +0.37(B-V), -0.01(U-B), F2V; vsini 30k/s. Delta Sct? Optical. Cst 6.4p. CP CygNashiraAlpha Cyg 4.69 - 4.78V. H alpha profile var. V337 CepBinary. Companion A3. AC fixed. C, 8.05V, +0.23(B-V), -0.68(U-B), B1.5V at 12", vsini 80k/s. AD also fixed. D, 8.03V, +0.20(B-V), -0.72(U-B), B2IV at 20", vsini 270k/s. In earlier sources C is brighter than D. Unlikely that this system is related to the X-ray source Cep X-4. AB binary. B, 10.5v at 3". Component C, optical. CPM. Suspected occultation double. Amp. 0.010V, 0.02B, 0.064d. CG OctSuspected occultation double. Lb 5.6 - 7.0v. Formerly called DS Peg, now in Cyg. V460 CygSRb 5.9 - 7.1v, 35?d. V1339 Cyg6.4 B9.5V, 6.6 A0V, 27.2y, a = 0.16". ADS 15251 8.3, 8.3, 11.9m at 2' may be member of same system. AzelfafageAB CPM. B is A0. AP, 5.6 11.0v sep. 1.5" binary. Enif represents the nose of [X/Pegasus]. This slightly reddish star is 540 [G/light year]s away and over 5,000 times more [G/luminous] than our [G/Sun]. ADS 15268AB optical. 0.7 - 3.5V. 1.7m flare 1972 Sept. 26-7; fainter than normal following night. ENIFAB 4.78 F4V, 6.09 G2V, 507.5y, a = 4.278". B is HR 8310. Combined colors. Mag. for blend 4.50V. Components C, D, optical. D, at 201" is ADS 15275, 6.9 A5, 13.3v sep. 16". Amp. 0.02V, 24.90d. Var. due to star spots? Period corresponds to period of rotation. Variable H and K emission indicates chromospheric activity. HN PegAB 4.7 F2IV, 5.0 F6IV, 11.558y, a = 0.255". ADS 15281C, 10.8v at 13.8" possibly in hyperbolic orbit about AB or is optical. ADS 15271A, SRc 3.43 - 5.1v, 730d; also a cycle of 4400d. Mean magnitude varies 13.5y. Correspondence between polarization and light. Herschel's "GarnSRb 5.90 - 6.14V, about 25d. AG CapADS 15314A. Component A is SB, 3.2, 5.2v, 0.0018"; B, 15.8v, 69"; C 12.7v, 120". EA (possibly RS CVn type) 2.83 - 3.05V, 1.0227789d. Form of light curve varies. Deneb AlgediSep. 0.102". Alpha Cyg 4.25 - 4.35V, 7.6:d. 5.5 F2, 7.5, 29.0y, a = 0.396"; previous orbits 37.594y, a = 0.433" and 27.508y, a = 0.387". Delta Sct? Both components optical. Alpha CV, amp. 0.01V, 20.70d. Double wave curve. Amplitude var. V1619 CygI, amp. 0.4B. HO Peg6.6 F0IV, 6.7 F0IV, 27.5y, a = 0.240". Combined mag., color. Occultation third component 8.8v at 0.02"; AB, sep. 0.114" by Finsen, 0.090-0.093" by speckle interferometry. AB CPM. B is A1p Sr Si, vsini 60k/s. C, 13.2v at 55". ADS 15405A, Beta C?, 5.68 - 5.71V. Component B Am(A2/A6/F2). Optical. AB CPM. Companion F7V. Delta Sct 6.13 - 6.21V, 0.147825d; also 0.11983 and possibly 0.14129 and 0.2172d. BZ Gru5.1 F0IV, 5.1 F0IV, 6.094y, a = 0.127", or 12.242y, a = 0.160". Combined mag., colors. EA 6.11 - 6.36V, 1.464047d, amp. 0.20 in uvby system. Similar spectral types both components, vsini 70k/s and 50k/s. H alpha profile variable. Identified in BAA* var. M2Iab, B6IIe. Combined mag., colors. Absolute magnitudes based on astrometric and spectroscopic data are -4.0V for red component, -2.3 for the blue. EA 4.80 - 5.36V, 6.65 - 7.46p, 7430d. Also slow oscillations, amp. 0.15, per. 13.7y and amp. 0.03, per. 349d. Red observations indicate Sr amp. 0.4m, 58d. H alpha varies in 118.37d, period stable over 20y interval. This is probably the pulsation period of the red component. Amplitude varies in period 825d or more. The blue companion may be intrinsically variable. VV Cep also magnetic variable. VV CepCompanion HD 208971, 7.0, K5III-IV, probably optical. Component B, 7.2v, at 3.7" variously classified G2V, G2III:, K0III:; C 11.7v at 143". ADS 15562A, EA 6.37 - 6.78V, 0.9450132d. DX AqrSecondary of visual double, 8.6 - 11.0v? Optical pair? Gamma Cas 4.68 - 4.89V, 4.57 - 4.65p. Ell 5.56 - 5.66B, 3.070510d. Identifed as Mu AB CPM. V1942 CygHe 10830 possibly variable. SADALMELIKLb? 5.13 - 5.33V. MO CepAB 4.61 A3m, 6.5 F7V or F3III-IV, 3800y, a = 11.5". Aa, 2.254y, a = 0.073". Component B is HD 209791 = GC 30876, vsini =<25k/s. Component C, 12.7v at 97" optical. AlkurhahSRb 6.08 - 6.36V, 82:d. HT LacAB binary. ALNAIR0.05V, 2.25d. Amp. 0.08V, 2.1727d. V365 LacCompanions optical: B, 11.6v at 20"; C 10.79V, +1.08(B-V), +0.75(U-B). Optical. 6.3 - 7.7:v. Old disk population runaway star. Emission variable in period over 50y. EA 6.08 - 6.77V, RS CVn-type binary, 1.98319204d (period changes). Distortions in light curve possibly due to star spots or to gas streams. Strong radio flare activity. AR LacComponents B and C optical. Delta Sct? BahamPossible nearby star on basis of spectroscopic parallax. B and C optical. D, K0, CPM. Polarization variable in intervals of about a day. AB optical. CPM. Probably single. AB binary. B is F8V. SRb 4.58 - 5.30V, about 55d. Also called BO Oct. B, optical. CPM. Companion A3V. Delta Sct 4.15 - 4.20V, 0.04242 and 0.068073d. Period and amp. vary. AnchaA* 2.85 K3III, 11.5y, a = 0.049". AB binary. AB CPM. B, 10.7v A7V at 6"; C, F6IV, optical. Sep. 0.100". Optical. SadalachbiaAmp. 0.43V. Emission var. period about 8y. IN PegCompanion G0V. B-V for combined light +2.10. Since 1900 no relative motion of components observed. Component A of visual double, SRb 5.41 - 6.70V, about 150d. Visual companion is optical. ADS 15862A, Ell?, 4.53 - 4.56V. CPM. Suspected occultation double. Unresolved by speckle interferometry. AB binary. B, 9.2v at 2.5" in 1832; 0.296" by speckle interferometry on 1985.5. AB 6.6 A0, 6.6, 190y, a = 0.490". Measured sep. 0.121" on 1985.5 by speckle interferometry. Gamma Cas 4.42 - 4.70V. Variable magnitude, RV and emission lines due to slow rotation of line of apsides of rapidly rotating equatorial shell. Spectrum variable 0.087d. Variable polarization. CPM companion F5III, optical. See HR 8544. Colors for combined light. Mag. of blend 5.56V. AB binary. B is K4. Fixed. Binary with HR 8559, speckle interferometric sep. 1.672" (1982.38). B* 4.51, 12v, 25.5y, a = 0.072". Companion optical. B-V for combined light +1.57. Lb? 3.99 - 4.20V. Del2 Gru5.77 F5IV, 7.14 F7IV, 143.0y, a = 0.746" or 140.0y, a = 0.75". Combined mag., colors. B, 13v at 21" optical. AC CPM, C at 41", 6.30V, -0.03(B-V), -0.35(U-B), B7IV, RV -21k/s, vsini 135k/s. ADS 15987A, CDelta 3.48 - 4.34V, 5.366341d. Period varies. Prototype star Delta Cep, discovered by Goodricke in 1784. Blue companion ADS 15987C is also var. and SB. Ell 6.27 - 6.47V, 17.748d, double wave light curve; mean mag. varies. V350 LacCPM. Companion D G2? Photometric data (Oblak 1978, A&AS, 34, 453) give B A2V, 6.22V,; C F2V, 7.71V, +0.38(B-V); D F9V, 7.83V, +0.51(B-V), where MK types are estimated from uvby,beta photometry. ABD physical, C optical. Delta Sct 6.30 - 6.32v, 0.056d. GX PegOptical. Al Kalb al RaiL, 5.8 - 6.8v, period about 1y. AB 6.5 dF2, 7.0 A5, 225.6y, a = 0.78", or 785y, a = 2.042". Combined colors; combined mag. 6.01V. Combined spectrum A9III. AB, CPM. CPM. AB CPM. B is 6.46V, -0.14(B-V), -0.82(U-B), B2V, vsini 40k/s. All companions listed by Worley are more than 22" from A. A new companion at 0.042" discovered by speckle interferometry. ADS 16095A, 4-10y cycles. Emission var. period 16-18y. Probably single. SitulaDelta Sct 6.62 - 6.68V, 0.12477d; also possibly 0.09466 or 0.08646 or 0.07956d and 0.07697d. CC GruMeasured sep. 0.136" on 1985.5 by speckle interferometry. ADS 16130. Uncertain which component varies, B-A 0.5 - 1.8v. ABC CPM. BC 7.3v F6IV, 8.1v sep. 3". Optical. Companion 10.02V, +0.28(B-V), +0.3(U-B), A6III-IV, vsini 141k/s. Optical. AB, 6.4 F8, 7.4 F6, 28.0y, a = 0.17". Speckle interferometric sep. 0.184" on 1985.5153. Occultations indicate third fainter component: sep. 0.129", mag. diff 2.7v 9 Oct. 1973; single 3 Dec. 1973; and 0.065", mag. diff 1.0, 29 Sept. 1974. Possibly variable with high orbital motion? AB 6.26 G3V, 6.81 G8V, 20.93y, a = 0.30". Combined mag., colors. Perhaps invisible companion, period 15.8y. ADS 16173C, 11.6v at 72". Faint CPM, 14.9v at 4.5' N. prec. HomamBinary. B is M1. Primary of visual double, 5.97 - 6.02:V, 6.43 - 6.53p. Variability doubtful. Lc? 2.0 - 2.3V. 6.05 - 6.08V, variability doubtful. B, 9.2A3V, physical, vsini 89k/s. Beta C 5.16 - 5.28V, 0.1930924d. Six secondary periods reported, ranging from 0.095109 to 0.23583d. DD LacAB binary. B9, A7. A* 2.94 G2II-III, 2.23y, a = 0.022". Speckle interferometry measures range from unresolved to sep. 0.059". BC, 10.0, 10.0v sep. 0.2" at 90" from A, physical. ADS 16211A. MatarBC, 7.6, 9.5v sep. 0.15" binary and AxBC binary. Uncertain which component varies. AB binary. B is K2III. C, 12.5v at 11" optical. Fixed sep. CPM, companion G9V. AB binary. B 12v M1 at 12"; C, optical. Delta Sct?, amp. 0.01V, 0.052:d. AB optical. Delta Sct 6.16 - 6.19V, 0.087d. FM Aqr7.0 F2IV, 7.2 F3IV, 26.9y, a = 0.212". Combined mag., color. Old disk population runaway star. AB binary. B is dF5. A is astrometric binary, 4.3y. C is 10.2v at 111". EB 5.91 - 5.98V, 10.075d. Detached main sequence stars. V360 LacBinary, companion F5V. AB binary. B is G2IV. Combined mag., colors. CPM companion M4. Lb 3.70 - 3.80V. AB, CPM. B, 12.2v at 26". Tau1Amp. 0.16V. Out of phase with orbital period. IM PegMag., colors for combined light. Occultation double 6.7, 6.7v sep. 0.2"; speckle interferometry, sep. 0.076". Alpha CV, amp. 0.005V. Possible periods 0.724, 1.27, 3.40, 1.70d. HI AqrAB 5.8 A3VM, 7.8 F6V, 104.5y, a = 0.647", or 102.27y, a = 0.680". Component C, optical. SkatAmp. 0.2:V, 50:d. HR Peg120.0y, e 0.68, a 0.47", i 85d, mag. diff 2.0. ADS 16365B, 7.6v. CPM. Companion G3. CPM with HR 8728. BY 6.44 - 6.49V, 10d. TW PsAAB relative position of component unchanged in a century. Probably physical. B, 11.5v F0 at 27". C, F5IV, optical, vsini =<54k/s. ADS 16381A, Beta C, amp. 0.11B, 0.169170, 0.170770 and 0.181692d. Also EA, amp. 0.04V, 12.096816d. EN LacAmp. 0.06V. Fomalhaut is a bright, white star that lies only 22 [G/light year]s away. Its diameter is twice that of our [G/Sun] and it is 14 times more [G/luminous]. CPM with HR 8721. FOMALHAUTGamma Cas 5.22 - 5.48V, 5.0 - 5.3p; later observations 5.15 - 5.21V. Amp. variable. Periods at different times have varied from 0.7364 in 1951 to between 0.800 and 0.700d; more recent periods were a choice in 1980 between 0.725 and 0.418d; 0.711 in 1981 and then 0.722d. Also indications of long-term changes. Spectrum variable 2.4 - 10.8y. Spectrum also indicates atmospheric quasi-periodic pulsations of about 1d. Strong spectrum and color changes in 1978. EW LacSep. 0.02", but duplicity uncertain. Unresolved by speckle interferometry. AB 7.1 G2V, 7.3 G4V, 26.5y, a = 0.39". Combined mag. ADS 16417AB varies slightly. 6.1 F0V, 7.4 F6V, 270.13y, a = 0.815". Combined mag., colors. Delta Sct? Amp. 0.018V, pulsating. Radio source. One of the most luminous stars in the galaxy. Circumstellar gas shell. Circumstellar features observed in infrared. SRd 4.75 - 5.50V. Spectrum variable. Variable NII emission. Probable nonradial pulsations coupled with mass loss. Phase between V and B-V curves changed between 1980 and 1985, from half phase out of cycle to in phase. Cycles on time scale of about a year. Bimodal radial pulsation inferred (Sheffer and Lambert 1987, PASP, 99, 1277) from analysis of a decade of spectroscopic observations. As opposed to remarks on spectral type, the star appears to be getting bluer (IBVS 3170), implying an increase in temperature of 800 K over the past decade. V509 CasCPM. Gamma Cas?, 6.53 - 6.60V. Suspected occultation double. Separate speckle interferometric measures give sep. 0.05" (Aa) and 0.34" (AB). Ten years of observations reveal steady change in AB position angle of about 10d with decrease in separation from about 0.375" to 0.266". Component B identified as SB2 (see SB remarks), making total number of components at least 4. Gamma Cas 3.58 - 3.65V. Photometric investigations have indicated numerous periods, particularly 0.78823, 1.0815d and 1.5998398d, all doubtful. Form of light curve varies. Probably not an eclipsing binary. Period shell phenomena about 23.5y. Shell features have vanished several times since 1897. H gamma varies in 3.66?d. AB 5.1 A2, 8.8, 76.6y, a = 0.277". ADS 16467B, Delta Sct?, 8.7v. Cst? 5.11V. Fixed. Companion 9.88V, +0.08(B-V), -0.37(U-B), A1V. Amp. 0.02b, 35 min. LN AndAlpha CV, amp. 0.10u, 5.36d. Spectrum variable. V638 CasFum al SamakahLb 2.31 - 2.74V. SCHEATBinary questioned. Companion 9.47V, +0.09(B-V), -0.20(U-B), B9V. The star Markab makes up the southwest corner of the Great Square of [X/Pegasus]. It is 86 [G/light year]s distant. MARKABAB 6.2 F2Vn, 6.3 F2V, 21.84y, a = 0.200" or 22.0y, a = 0.20". Combined mag., colors. Component C, 84 Aqr, 7.6v K0 at 262", optical. Sep. 2.9" observed 1925; single in 1929. CPM. Combined mag., color. Companion F8V. Binary. ADS 16519. Uncertain which component varies, if either. Possible delta Sct type. Amp. 0.08V. Sep. 0.180". ADS 16550A, Lb? 5.0 - 5.16V. GZ PegAmp. 0.22V. AB 4.6 G2III, 6.6 F3V, 150y, a = 0.86". Combined mag., colors. Companion may be collapsed star. C, 8.14V, +0.15(B-V), -0.38(U-B), A, HD 218780. ADS 16556A. Astrometric binary unresolved by speckle interferometry. Amp. 0.02B. Probably optical. AB, CPM. BC, 10.0, 10.5v, K3V, 130y, a = 0.6", mean mass BC 0.35 solar. BC combined, 9.19V, +1.03(B-V), +0.93(U-B), CPM with A. Component C is a close double, equal components, showing orbital motion. Lb 4.9 - 5.25V, 6.5 - 6.8p. High space velocity? E, amp. 0.08V, 0.09B. Close to X-ray source 4U2316+61. V649 CasSuspected occultation double. AB, CPM. B, 13.0v at 8". Alpha CV 6.48 - 6.50V, larger amp. in U = 0.05, 0.617135d, 0.49925d. Other periods previously determined range from 0.44925 to 2.604d. Spectral line strengths vary but not in phase with orbital (SB) period. ET AndEB 6.0 - 6.16p, A7+A, 3.219565d. AN AndAB binary. ADS 16671B, 9.0 - >12?v. AB binary. B is K2V. Component A found double by speckle interferometry. CPM. AB 4.86 K0III, 7.13 F6V, 796.16y, a = 2.991". AB 6.04 F6III, 8.89V, +0.61(B-V), +0.08(U-B), G0V. AB CPM with C, 8.87v A3 at 17". Suspected occultation double. Delta Sct 4.60 - 4.62V, 0.05433d, secondary 0.04895d, beat period 0.4943d. SalmCPM. Amp. 0.14V. 5.6 A2V, 6.4 A7V, 63.16y, a = 0.420". Interferometer double. CPM. Companion A3III, vsini 129k/s. AB optical. Component A suspected occultation double. Alpha CV 4.91 - 4.96V, 0.58525:d. Period changes? Magnetic and spectrum variable, 0.5805d. Probably single star. Amp. 0.012V, 6.97d. HV PegAmp. 0.064v, 2.32d. Spectrum variable, especially SiII and SiIII. CG TucAB, 4.9, 9.3V, 1500y, sep. 1.1". CD, 8.2 A0Vn, 9.8v, sep. 1.6"; vsini of C, 210k/s. Component E, optical. ADS 16795A, EA 4.84 - 4.98V, 6.0663309d; i 90d. AR CasAmp. 0.06V. Alpha CV? 4.36 - 4.39V. Spectrum binary unresolved by speckle interferometry. 7.0 - 7.30p. HW Peg5.6 K4III, 5.7 K5III, 241.20y, a = 0.447". ADS 16836. Uncertain which component varies. Alpha CV 4.70 - 4.75V, about 12.5d. Magnetic variable. Duplicity questionable. Components K2.5IIIb and F9V. Confusion among RS 3.69 - 3.97V, 4.74 - 5.13B, 54.20d. Amp. and cycle length vary in period 3200d. Also 0.25m var. in period about 50d. H and K emission correlated with 56d light period. AB 6.3, 7.2v, 351.22y, a = 0.41". Ellipsoidal var, amp. 0.08B. Period consistent with SB. KS PegOptical. CPM. AlraiAB optical. Amp. 0.05(B-V). Delta Sct? Component B, CPM, A5Vep; however, the companion is optical. Amp. 0.05V. CPM, F6IV and G8V. 11813y, a = 14.21". Companion F2III or F2V, sources discordant; vsini 96k/s. Component A has composite spectrum but star unresolved by interferometer. vsini of G5 component <19:k/s, A0 component =<50k/s. Component B, 14.6v at 25"; C, 13.1v at 62". Lb 6.9 - 7.7p. TX PscADS 17006. Uncertain which component varies. AB binary. B, 11v at 4". C is HD 223340, G type. AC, CPM. AB 6.8 A0, 7.4v, 565.77y, a = 0.74". C, 8.6v at 50" optical. 0.9135 or 1.092d. Amp. 0.03u. V650 CasAB binary. B is cA0. Alpha Cyg 5.34 - 5.45V, =>46d. V566 CasRS CV, amp. 0.04V, 23.25d. OU AndLb? 5.74 - 6.0V. HH PegAlpha CV 5.16 - 5.21V, 3.730d. Variable magnetic field and spectrum. ET AqrAB binary. B, 12v M2 at 5". Delta Sct, amp. 0.01V, 0.06d. HT PegSep. 0.107". Companion F2V; vsini 43k/s. Components also classified A = Am(A1/A8V/F0), B = Am(A1/F1/F0). Possibly wide CPM pair with HR 9052. SRd 4.1 - 6.2v, periods about 110 and 1100d (1946 minimum lasted 320d). Rapid spectral variation from cF5 to M5p. Photoelectric observations since June 1986 indicate an amp. of only about 0.8V and 0.3(B-V). Rho CasLb 5.55 - 5.97V. XZ PscE 6.06-6.30V, B6, B9, 2.445094d. AL SclWide pair with HR 9045. E:/GS 5.9 - 6.3v, 13.4192d. Intrinsic variable which may be eclipsing. V373 CasCst? 6.6p. V CepE?, amp. 0.05V. 4.63 - 4.69V. ADS 17137B, 9.0 - 11.5V. Beta C? 6.4 - 6.46B, 0.310049 or 0.622832d. Spectrum variable. LQ AndAB binary, 5.0v B2III, 7.1v B3V. Binary with HR 9074, q.v. Probably single. Alpha CV 6.32 - 6.42V, 3.73975d, possible cyclical changes. Also magnetic field and spectrum period. Light var. also 2.1 hrs. Widths of hydrogen lines in about 35 min. SiII var. in per. 4.88643d. CG AndAB 5.84 G3V, 8.88 K6V, 26.386y, a = 0.803". A possible new companion found by speckle interferometry. Components C, D probably optical. C is K7V. Lb? 4.35 - 4.41V. YY PscADS 1B, 7.47V, +0.08(B-V), +0.05(U-B), A2Vn, vsini 275k/s, may be shell star. AB binary. C, 10.8m at 99" optical. I? Amp. 0.1B. V639 CasBinary. Amp. 0.02:V, 6.4322d. V567 CasThe [G/constellation] Andromeda is named for the mythical daughter of King [Y/Cepheus] and Queen [Y/Cassiopeia]. To save their kingdom, Andromeda's parents were told they must sacrifice their daughter to the sea monster, [Y/Cetus]. Andromeda was chained to the rocks by the sea to await her fate. Fortunately, [Y/Perseus], riding the winged horse [Y/Pegasus], flew over the kingdom. He saw the princess chained to the rocks and flew down to rescue her. In the sky, Andromeda is shaped like the capital letter "A" with her head at the point of the "A", her belt at the central line of the "A" and her feet at the base of the "A". Her brightest [G/star] is [W/Alpheratz], the star at the top of "A" and one of the stars in the Great Square of [Y/Pegasus]. Andromeda is best seen from October-December. "Must See" objects include: [F/Andromeda Galaxy]; [N/NGC 752], a star [G/cluster]. Antlia is a relatively modern [G/constellation]. It was added to the charts in 1752. This is a faint constellation, with no stars brighter than [G/magnitude] 4.2. Its brightest [G/star] is Alpha Antlia ([S/201405]). Antlia is best seen from April-June. Apus is a faint [G/constellation], with 5 of its 6 brightest stars reddish in color. The brightest [G/star] in Apus is Alpha Apodis ([S/257193]). This constellation is best seen from May-August in the southern hemisphere. The [G/constellation] Aquarius is associated with water in the mythology of many cultures, perhaps because Aquarius rises during autumn in the northern hemisphere - the rainy season for many countries. In Greek mythology, Aquarius caused a great flood that covered the Earth. To the Egyptians, Aquarius poured water into the Nile river each year, causing it to flood. The brightest [G/star] in Aquarius is Sadalsuud [S/145457]. Four stars make up the "Water Jar" of Aquarius: three stars forming a triangle with a fourth star in the center. Stars representing water are pouring from the jar. Aquarius is best seen from September-December. "Must See" objects include: [M/M2], a star [G/cluster]; the [F/Saturn Nebula], a [G/planetary nebula]; [F/Helix Nebula], a [G/planetary nebula]. In Greek mythology, Aquila was the eagle who served Zeus. Aquila carried the god's thunderbolts and delivered messages for him. In Chinese legends, the brightest [G/star] in Aquila, [W/Altair], represented one of two lovers in the tale of the herd boy and the weaving girl. Altair was the hard working herd boy, who fell in love with the weaving girl, a beautiful visitor from the stars. In the sky, three stars form the head of the eagle; Altair is the center star with a fainter star on each side. This [G/constellation] lies along the [G/Milky Way]. Look for dark lanes of dust (areas with fewer stars) in this region. Aquila is best seen from August-October. Ara is a modern [G/constellation] lying just below the curving tail of [Y/Scorpius]. Its brightest star is Beta Arae [S/244725]. Ara is best seen from July-September in the southern hemisphere. In Greek mythology, Aries was a ram with a beautiful golden fleece. This golden ram was identified with Zeus, the king of the gods. In Egyptian mythology, the celestial ram was thought to be Ammon, the Sun god. This faint [G/constellation] was identified with the bright Sun and shiny gold because of its location along the [G/zodiac]. Ancient people noted that when the [G/Sun] was in the constellation of Aries, this marked the beginning of spring and the growing season. Its brightest star is [W/Hamal]. Today, Aries is best seen from October-February. Auriga is a strange [G/constellation], representing a charioteer who is carrying a goat on his shoulder and holding three baby goats in his arms. The brightest [G/star] in Auriga is [W/Capella]. The three baby goats, also known as "The Kids," are represented by three stars forming a narrow triangle, just south of Capella. Auriga is best seen from January-March. "Must see" objects include: three galactic [G/cluster]s, [M/M36], [M/M37], and [M/M38]. Bootes was placed in the sky to guard the great bear, [Y/Ursa Major]. As a result, Bootes can be seen following the bear around the sky once a day. The brightest star in Bootes, [W/Arcturus], can be found by using stars in the [G/Big Dipper] to point the way. If you connect the three stars in the handle of the Dipper, this forms an arc. Follow this arc to Arcturus. Bootes is shaped like an ice cream cone, with Arcturus at the tip of the triangular cone. Two stars finish the cone and there is a small scoop of ice cream on top. Bootes is best seen from June-August. Caelum is a small, faint constellation with no [G/star]s brighter than [G/magnitude] 4.5. Its brightest star is Alpha Caeli [S/216926]. Caelum is best seen from January-February. Camelopardalis was added to the charts in 1690. There are no stars brighter than [G/magnitude] 4.0 in this area of the sky. There is also no easy-to-identify pattern. Its brightest [G/star] is Beta Camelopardalis [S/13351]. This constellation is [G/circumpolar], meaning it is visible year round from most of the northern hemisphere. It is best seen from December-February. Cancer is the faintest of all the [G/constellation]s of the [G/zodiac] and is best viewed under dark skies when the [G/Moon] is not visible. In Greek mythology, Cancer the crab lived in a swamp with the [Y/Hydra]. When [Y/Hercules] came to kill the Hydra, Cancer tried to save his friend by biting Hercules on the foot. Hercules merely killed the crab and brushed it aside. Cancer was given a place in the sky, to honor him for sacrificing his life for a friend. The brightest [G/star] in Cancer is Altarf [S/116569]. This constellation is best seen from March-May. "Must See" objects include: the [F/Praesepe] cluster. The brightest [G/star] in Canes Venatici is [W/Cor Caroli] and it represents one of two hunting dogs in this [G/constellation]. Cor Caroli (the Heart of Charles) was probably named after King Charles I of England, but this bright star is usually associated with the coronation of King Charles II in 1660. The second hunting dog is represented by Beta [S/44230]. This constellation is best seen from May-July. "Must See" objects include: [F/Whirlpool Galaxy]; [M/M3], a globular [G/cluster]; [M/M94], a spiral [G/galaxy]. Canis Major, lying next to the mighty hunter [Y/Orion], is sometimes known as Orion's hunting dog. Its brightest star, [W/Sirius], is also the brightest [G/star] in the night sky and has been worshipped and feared by many cultures. In the past, Sirius (also known as the Dog Star) rose and set with the Sun during the hottest days of summer, causing it to be blamed for the scorching summer heat. As a result, the phrase "Dog Days of Summer" can be associated with this [G/constellation]. Canis Major is best seen in the night sky from February-April. "Must See" objects include: [M/M41], a galactic [G/cluster]; [N/NGC 2362], a galactic [G/cluster]. Canis Minor is the smallest of [Y/Orion]'s two hunting dogs. The brightest [G/star] in this small [G/constellation] is [W/Procyon]. Procyon forms a triangle with two other bright winter stars, [W/Sirius] and [W/Betelgeuse]. Canis Minor is best seen from February-April. Capricornus is one of the older [G/constellation], although its origin as a half goat-half fish is not clear. According to one Greek myth, Capricornus was Aegipan, a half man, half goat whose father was Zeus. Once, while helping his father, Aegipan was pursued by Typhon, the monster god. To avoid Typhon, Aegian ran into a river. When he was waist-deep in the water, he changed the lower part of his body into a fish and swam to safety. Zeus placed Aegipan in the sky, as a way of thanking him for his help. The brightest [G/star] in this constellation is Deneb Algedi [S/164644]. Capricornus is best seen from September-November. Carina, originally part of the ancient [G/constellation] of Argo, the ship, is best seen from the southern hemisphere. Its brightest [G/star] is [W/Canopus], the second brightest star in the night sky. ([W/Sirius] is the brightest.) Carina is best seen from March-May. "Must See" objects include three galactic [G/cluster]s: [N/NGC 2516]; [N/NGC 3532]; [C/C102]. In Greek mythology, Queen Cassiopeia, along with her husband, King [Y/Cepheus] ruled over Ethiopia. Cassiopeia was very beautiful, but boastful and arrogant as well. She once boasted that she was even more beautiful than the sea nymphs. This claim angered the sea nymphs, whose beauty was legendary. They complained to Poseidon, the god of the sea, who sent [Y/Cetus], a sea monster, to destroy Ethiopia. Cassiopeia and Cepheus were forced to sacrifice their daughter, [Y/Andromeda] to save their kingdom. Fortunately, Andromeda was saved by [Y/Perseus] and [Y/Pegasus]. Cassiopeia sits on her throne in the sky, with her brightest stars forming a "W" or "M" shape, depending on the season. The brightest [G/star] is [W/SHEDIR] which lies at the lower right vertex of the "W". Because of her placement in the sky, half the time her royal throne is upside down. The queen must be chained to the chair so she won't fall out. This awkward position is part of her punishment for being so vain. Cassiopeia is a [G/circumpolar] constellation and can be seen most of the year. However, she is best seen from September to December. "Must See" objects include four galactic [G/cluster]s: [M/M103]; [N/NGC 457]; [N/NGC 7789]; [N/NGC 663]. In Greek mythology, Centaurus was the first of the Centaurs, a race of beings with the head, arms and chest of a man and the body of a horse. The brightest [G/star] in this [G/constellation] is Alpha Centauri, [S/252838]. It is also the closest star to our solar system. Alpha Centauri along with Agena [S/252582] make up the "Pointers", two bright stars that point the way to the [G/Southern Cross]. Centaurus is best seen from May-July in the southern hemisphere. "Must See" objects include: [F/Omega Centauri], a globular [G/cluster]; [F/Centaurus A], a peculiar [G/galaxy]. In Greek mythology, King Cepheus ruled over the country of Ethiopia with his beautiful, but vain, wife [Y/Cassiopeia]. Cepheus was forced to sacrifice his daughter [Y/Andromeda] to save his kingdom from [Y/Cetus] the sea monster. As fortune would have it, Andromeda was rescued by [Y/Perseus] and [Y/Pegasus] and the sea monster was killed. Peace was restored to the kingdom. The stars in this [G/constellation] form a box with a triangle sitting on top. The brightest [G/star] in Cepheus is [W/Alderamin]. This constellation is [G/circumpolar] and can be seen most of the year. However, it is best seen from September-December. "Must See" objects include: [N/NGC 188], a galactic [G/cluster]. Cetus, the sea monster, was sent to destroy the kingdom of King [Y/Cepheus] and Queen [Y/Cassiopeia]. But, before he could complete his task, he was killed by [Y/Perseus]. The brightest [G/star] in the [G/constellation] is [W/Diphda]. Cetus is best seen from October-December. "Must See" objects include: [W/Mira], a variable star. Chamaeleon was added to the charts in the early 1600's and is considered a modern [G/constellation]. It is small in size and shaped like an elongated diamond. Its brightest [G/star] is Alpha Chamaeleont [S/256496]. Chamaeleon is [G/circumpolar] and can be seen most of the year from the southern hemisphere. This small, narrow "V"-shaped [G/constellation] lies close to the "Pointers", the two brightest stars of [Y/Centaurus]. Circinus is a modern constellation, added to the charts in the mid 1700's. It contains a few relatively faint [G/star]s, the brightest of which is Alpha Circini [S/252853]. Circinus is best seen from July-September in the southern hemisphere. The brightest [G/star] in this [G/constellation] is Phact [S/196059]. Columba is best seen from January-March in the southern hemisphere. "Must See" objects include: [N/NGC 1851], a globular [G/cluster]. Coma Berenices was named after Berenices II who, along with her king, ruled Egypt around the year 230 BC. With the king at war, Berenices offered to sacrifice her long golden hair to the goddess Aphrodite to insure the safe return of her husband. When the war was over, the king returned safe and sound and Berenice kept her promise. She cut her hair and left the golden tresses on an alter as a gift to the goddess. The next morning, the tresses were gone. Local astronomers convinced the king and queen that the golden tresses had been transported into the sky where they would forever sparkle among the stars. Today, the [G/constellation] consists of a scattering of faint stars, most of which belong to an extremely large galactic [G/cluster] known as the [G/Coma Star Cluster]. The brightest star in this constellation is Diadem [S/100443]. Coma Berenices also contains a wide assortment of galaxies. Unfortunately, most are too faint to be seen with a small telescope. Coma Berenices is best seen from May-July. "Must See" objects include: [M/M53], a globular cluster. Corona Australis is shaped like a "C" and lies just below the "Teapot" of [Y/Sagittarius]. The brightest [G/star] in the [G/constellation] is Alfecca Meridiana [S/210990]. Corona Australis is best seen from August-October. In Greek mythology, the god Bacchus created a beautiful crown which he gave to his mortal wife. Upon her death, he placed the crown in the sky as a tribute to his wife's great kindness and beauty. To the Shawnee Indians, the stars of this [G/constellation] represent celestial sisters. The circle of stars is incomplete because one sister left the sky to marry a human. The stars in Corona Borealis are shaped like the letter "C". Its brightest star is [W/Alphekka]. This constellation is best seen from July-September. In Greek mythology, Corvus was the messenger raven for the god Apollo. One of raven's many tasks included bringing water to the god when he was thirsty. One day, Corvus was about to fill a goblet with water when he noticed a fruit tree in bloom. He decided to wait until the fruit was ripe so that he could have a snack before returning to Apollo. Corvus waited several days for the fruit to ripen. Finally, he ate his fill of the ripe, fresh fruit and started back to Mount Olympus. Along the way, he realized that Apollo might be angry with him for taking so long to fetch the water. Thinking fast, he swooped down and snatched a water serpent from the river. Then, when he returned the goblet of water to Apollo, Corvus explained that the water serpent had attacked him, causing him to be late. Apollo did not believe the raven's story and flung the raven, the goblet and the water serpent into the sky where they would not bother him again. Today, the raven, or Crow (Corvus), the goblet ([Y/Crater]), and the sea serpent ([Y/Hydra]) are all constellations. The brighter stars of Corvus form a lopsided rectangle in the sky. Its brightest [G/star] is Gienah [S/157176]. Corvus is best seen from April-June. In Greek mythology, Crater represented a water goblet which belonged to the god Apollo. [Y/Corvus] the crow used the goblet to gather water for the god when he was thirsty. Crater was caught in the middle of a fight when Corvus tried to lie to Apollo. In a fit of rage, Apollo flung both the crow and the goblet into the sky. To many cultures, Crater represented a cup, bowl, or some other type of container used to hold wine. The brightest star in Crater is Delta Crateris [S/156605]. Crater is best seen from April-June. Even though Crux is the smallest [G/constellation] in the sky, it contains some of the richest starfields of our [G/Milky Way] galaxy. Originally, Crux was part of the constellation [Y/Centaurus]. Today, its brightest stars appear in the shape of a cross. The brightest star in Crux is [W/Acrux], a fine double star system. Crux is best seen from April-June. "Must See" objects include: [F/Jewel Box] cluster; [F/Coal Sack] nebula. Cygnus, which is also known as the Northern Cross, lies along the hazy patch of light that makes up our [G/Milky Way] galaxy. One Greek myth tells how Cygnus represents Zeus, the king of the gods. Zeus once turned himself into a swan to seduce the lovely mortal woman, Leda. Leda then laid an egg and when the egg hatched, the beautiful Helen of Troy was born. Another myth tells that Cygnus was the best friend of Phaethon. Phaethon had discovered that his real father was Apollo, the Sun god. He went to visit Apollo and watched as his father drove the Sun's chariot across the sky once a day, bringing daylight to the world. Phaethon demanded that he be allowed to drive the chariot, and before Apollo could stop him, he grabbed the reins of the chariot and took off. The four fiery horses pulling the chariot went wild and Phaethon lost control. To save Earth from the runaway Sun chariot, Zeus was forced to fling a lightening bolt and killed Phaethon. Phaethon's body plunged to Earth and fell into the river [Y/Eridanus] while the horses safely returned the Sun's chariot to Apollo. Phaethon's friend, Cygnus, searched the river, but he never found his friend. He continued swimming back and forth, diving deep into the river's depths, reminding those who watched him of a swan. For his devotion to his friend, Cygnus was honored with a place in the sky. Today, he can be seen as the swan flying south along the [G/Milky Way]. The [G/star] at the tail of the swan is also the brightest star in the [G/constellation]. Its name is [W/Deneb]. Cygnus is best seen from August-November. "Must See" objects include: [W/Albireo], a double star; the [G/Milky Way]; [F/Cygnus X-1], a black hole. To many cultures, the stars in Delphinus represented a dolphin or porpoise. In one myth, a dolphin rescued a man about to be killed by pirates. The man had jumped overboard and the dolphin helped him back to shore. For his good deed, the dolphin was honored with his own place in the sky. Five stars in the shape of a diamond form the dolphin's body, with two stars trailing off the diamond, forming the dolphin's tail. The brightest [G/star] in Delphinus is Rotanev [S/106316]. This [G/constellation] is best seen from August-October. Dorado was added to the charts in the early 1600's and is considered a modern [G/constellation]. Its brightest [G/star] is Alpha Doradus [S/233564]. Dorado is best seen from December-February from the southern hemisphere. "Must See" objects include: The [F/Large Magellanic Cloud], a [G/galaxy], the [F/Tarantula Nebula], a nebula within the Large Magellanic Cloud. In Greek mythology, Draco was the dragon in charge of guarding the garden of Hera, the queen of the gods. Within the garden, there were trees on which grew golden apples. [Y/Hercules] had to steal these golden apples as one of his 12 labors. Before he could steal them, however, he had to kill Draco. Draco fought a mighty battle, but he was no match for Hercules. After his death, Hera gave Draco an honored place among the stars. Three stars forming the tail of the dragon lie between the [G/Big Dipper] and [G/Little Dipper]. From the tail, Draco curls around the Little Dipper like a backwards "S". Its head is made up of four stars in the shape of a lopsided square. The brightest star in Draco is [W/Etamin] and it, along with the entire constellation, is best seen from July-September. "Must See" objects include: [W/Thuban], a star which was the "North" star 4,800 years ago. The stars of this small [G/constellation] may once have been combined with the stars of [Y/Delphinus] to form a larger constellation. However, the two were divided into individual constellations somewhere around the second century BC. Today, Equuleus lies between Delphinus and the head of [Y/Pegasus]. Its brightest [G/star] is Kitalpha [S/126662]. This constellation is best seen from August-October. Eridanus, the river, meanders all over the sky. In Greek mythology, it was this river that the body of Phaethon plunged into after his foolish ride across the sky in the chariot of the Sun. (You may refer to the constellation [Y/Cygnus] for the entire story of Phaethon.) Eridanus begins with the star Zaurak [S/149283], which lies next to the star [W/Rigel] in the constellation of [Y/Orion]. From there, Eridanus wanders below [Y/Cetus], around [Y/Fornax], above [Y/Horologium] and finally comes to an end between [Y/Phoenix] and [Y/Hydrus]. Its brightest star, [W/Achernar], lies so far south that it can't be seen from Europe, Japan and most of the U.S. This [G/constellation] is best seen from December-February. This small, faint group of stars is a modern [G/constellation] that was added to the charts in the late 1700's. Fornax lies next to [Y/Eridanus] in the sky. Its brightest [G/star] is Fornacis [S/168373]. This constellation is best seen from December-February. The stars in Gemini have been referred to as the "Twins" by many cultures around the world, with each culture offering a different story about the celestial brothers. One Greek myth tells that the twins are sons of Zeus, the king of the gods, and a mortal woman, Leda. The twins are also associated with "St. Elmo's Fire", an electric glow seen around aircraft wings or a ship's rigging during stormy weather. [W/Pollux], the brightest [G/star] in this [G/constellation], and a faint companion star form the head of one twin. The second brightest star in the constellation, [W/Castor], along with a fainter companion, forms the head of the second twin, with the twins standing side by side in the sky. Gemini is best seen from January-April. "Must See" objects include: [M/M35], a galactic cluster. Grus is a modern [G/constellation], added to the charts in the early 1600's. It is also part of a group of constellations known as the Southern Birds. The other birds of the group are the [Y/Phoenix], [Y/Pavo] the peacock, and [Y/Tucana] the toucan. The brightest [G/star] in Grus is [W/Alnair], a hot blue star. The second brightest star, Beta, [S/231258] is a cooler, orange-colored star. Compare the two and try to detect the differences in color. Grus is best seen from September-November in the southern hemisphere. Hercules was the son of Zeus, the king of the gods, and a mortal woman, Alcmene. Even as a young child, Hercules possessed a tremendous strength. When he was 8 months old, he strangled 2 serpents that had been sent to his crib by Hera, the jealous wife of Zeus. Hera's jealousy was to haunt Hercules for most of his life. At one point, she caused him to go insane. During this time of madness, Hercules killed his wife and children. When he awoke from the insanity, he saw the horror of what he had done and was overcome with grief. He left his village and traveled to the Oracle of Delphi for advice. The oracle told him to travel to Tiryns where King Eurystheus would assign Hercules 12 difficult labors. If and when Hercules completed all the labors, he would be freed from his sins and raised to the rank of godhood. For many years, Hercules struggled to complete the 12 labors, each more difficult than the last. Some of his opponents can be found in the sky, including [Y/Leo], the lion; [Y/Hydra], the many-headed serpent; [Y/Cancer], the crab; and [Y/Draco], the dragon. After many years, he successfully completed the 12 labors. When Hercules died, the gods welcomed him to Mount Olympus, where he was granted godhood, just as the Oracle had foreseen. Today, Hercules can be found next to the head of Draco. Four stars make up the "Keystone", or body of the mighty warrior. The brightest [G/star] in the [G/constellation] is Kornephoros [S/84411]. Hercules is best seen from July-September. "Must See" objects include: two globular [G/cluster]s, [M/M13] and [M/M92]. This small, faint group of stars is considered a modern [G/constellation], added to the charts in the 1700's. Its brightest [G/star] is Alpha Horologii [S/216710]. Horologium is best seen from December-February in the southern hemisphere. Hydra is the largest [G/constellation] in the sky. Its stars snake across over one quarter of the heavens. This constellation figures prominently in two Greek myths. In one myth, Hydra was a many-headed monster who lived in a swamp, along with her only companion, [Y/Cancer] the crab. [Y/Hercules] was sent to kill the monster as one of his twelve labors. The two fought a tremendous battle. For every head Hercules chopped off, Hydra grew two more in its place. Finally, Hercules won and the gods placed the body of Hydra in the sky. In another myth, Hydra was an innocent water serpent who was scooped out of a river by [Y/Corvus] the crow. The brightest [G/star] in Hydra is [W/Alphard]. Because Hydra is such a long constellation, various parts of it can be seen beginning in March and stretching through August. "Must See" objects include: [M/M48], a galactic [G/cluster]; [M/M68], a globular cluster; [M/M83], a spiral [G/galaxy]. This modern [G/constellation] was added to the charts in the early 1600's. Its brightest [G/star] is Beta Hydri [S/255670]. This star is the closest bright star to the south [G/celestial pole], even though it is over 12^ away. Hydrus is a [G/circumpolar] constellation and can be seen most of the year in the southern hemisphere. However, it is best seen from December-January. Indus is a rather small, faint [G/constellation] which lies next to the brighter constellation of [Y/Grus]. Its brightest [G/star] is Alpha Indi [S/230300]. Indus is best seen from September-November in the southern hemisphere. Lacerta is a relatively modern [G/constellation], added to the charts in 1690. It is a small, faint group of stars not far from the constellation of [Y/Cygnus]. The brightest [G/star] in Lacerta is Alpha Lacertae [S/34542]. The lizard's head is made up of four stars in the shape of a diamond. A trail of faint stars coming off the diamond forms the lizard's body. Lacerta is best seen from September-November. In Greek mythology, Leo is associated with the Nemean lion, a fierce creature who came from the Moon. [Y/Hercules] was given the difficult task of killing the ferocious beast. The lion's hide was so tough, no weapon could pierce through it. Arrows that Hercules flung at the beast merely bounced off its chest. Abandoning his useless weapons, Hercules trapped the lion and used his own incredible strength to strangle the creature. The lion's body was then placed in the sky by Hera, the queen of the gods and an enemy of Hercules. The [G/constellation] of Leo has long been associated with the [G/Sun] and hot summer days because, for 4,000 years, the Sun rose in this area of sky on the Summer [G/Solstice], the first day of summer in the northern hemisphere. Today, because of the [G/precession] of the Earth, Leo rises with the Sun in late July and early August. In the sky, the head, mane and chest of the lion are represented by a pattern of stars in the shape of a sickle or backwards question mark. The [G/star] at the handle of the sickle, or the "period" of the question mark, represents the heart of the lion. This star, called [W/Regulus], is the brightest star in Leo. The lion's hindquarters are represented by a small triangle containing [W/Denebola], a bright star whose name means the "Tail of the Lion". Leo is best seen from March-June. "Must See" objects include: two spiral galaxies, [M/M65] and [M/M66]. Leo Minor was added to the charts in 1690. It is a small, faint [G/constellation] that lies between the scoop of the [G/Big Dipper] and the sickle of [Y/Leo]. Its brightest [G/star] is Praecipua [S/62297]. Leo Minor is best seen from March-May. This little hare lives a rather hectic life, positioned in the sky next to a big dog, [Y/Canis Major], and just below the feet of the mighty hunter, [Y/Orion]. Its brightest star is [W/Arneb]. Lepus is best seen from January-March. Of all the [G/constellation]s of the [G/zodiac], Libra is the only one that does not represent a living being. However, the name of its brightest star, Zuben Elschemali [S/140430] (which means the northern claw) indicates that this area of sky was once part of the constellation of [Y/Scorpius]. Libra is best seen from June-July. Lupus is one of the original 48 [G/constellation]s placed in the sky by the ancient astronomer, Ptolemy. It contains several bright [G/star]s, but no easy-to-identify pattern. Its brightest star is Alpha Lupi [S/225128]. Lupus is best seen from June-July. The faint [G/constellation] of Lynx was added to the charts in 1690. Its brightest [G/star] is Alpha Lyncis [S/61414]. Lynx is best seen from February-April. "Must See" objects include: [N/NGC 2419], a globular [G/cluster] In Greek mythology, Lyra represented a beautiful lyre which had been fashioned from an empty tortoise shell. Orpheus, the son of Apollo, inherited the lyre from his father. When Orpheus played the lyre, his music was so beautiful it was said to charm anyone who heard it. Orpheus fell in love and married the beautiful Eurydice. The two lovers were extremely happy, but soon after their marriage, Eurydice was poisoned by a snake and died. Orpheus' grief was overwhelming. He took his lyre to the edge of the Underworld, where all mortal souls go when they die. There, he played his music. The Lord of the Underworld was so touched by the mournful sounds, that he allowed Eurydice to return to the land of the living. There was one stipulation, however. Orpheus could not look at Eurydice until they had completely left the boundaries of the Underworld. As the two lovers made there way back to the surface, Orpheus tried his best not to look at his wife, but the temptation was too great. Just as they neared the boundary between the two worlds, he glanced in her direction. Even a glance was too much and Eurydice was pulled back into the Underworld, never to return. For the rest of his life, Orpheus grieved over the loss of his wife, playing mournful, beautiful music on his lyre. After his death, the gods immortalized his music by raising the lyre into the stars. In one Chinese legend, Lyra's brightest [G/star], [W/Vega], represents one of two lovers from the tale of the Herd Boy and the Weaving Girl. Vega was the Weaving Girl, who wove beautiful tapestries among the stars. An interesting note about Vega: due to the [G/precession] of Earth's rotation, Vega was the "north" star 12,000 years ago, and will be again in another 12,000 years. Lyra is best seen from June-September. "Must See" objects include: the [F/Ring Nebula], a planetary nebula; Epsilon Lyra ([S/67310]), a double/double star; [M/M56], a globular cluster. This small group of stars holds the record for being the faintest of all the [G/constellation]s in the sky. None of the [G/star]s within this group are brighter than [G/magnitude] 5. In fact, its brightest star, Alpha Mensae ([S/256274]) is only magnitude 5.1. Mensa is a [G/circumpolar] constellation and can be seen year round from the southern hemisphere. "Must See" objects include: a small portion of the [F/Large Magellanic Cloud] that extends into this constellation. Microscopium is a faint, modern [G/constellation], added to the charts in the 1750's. Its brightest star, Gamma Microscopii [S/212636] is only [G/magnitude] 4.7. Microscopium is best seen from September-October in the southern hemisphere. Monoceros was added to the charts in the mid 1600's. Although faint, this [G/constellation] is rather easy to find. Simply form a triangle with three bright neighboring stars, [W/Betelgeuse], [W/Sirius], and [W/Procyon]. The area inside the triangle is Monoceros. The light from the brightest [G/star], Beta Monocerotis [S/133316], is actually the combined light from three different stars, one of the best triple star systems in the sky. Monoceros is best seen from February-March. "Must See" objects include: the [F/Rosette Nebula]; [N/NGC 2264], a Christmas-Tree-shaped cluster and nebula; [M/M50], a galactic cluster. This [G/constellation] was first listed on the charts in the early 1600's as a Bee. It was transformed to a fly in the mid 1700's. Musca lies between [Y/Crux] and the south [G/celestial pole]. Its brightest [G/star] is Alpha Muscae [S/251974]. Musca is a circumpolar constellation and can be seen year round in the southern hemisphere. However, it is best seen at sunset during May-June. "Must See" objects include: two globular [G/cluster]s, [N/NGC 4833] and [N/NGC 4372]. Norma is a faint [G/constellation] that was added to the charts during the 1750's. It is best seen during July-August from the southern hemisphere. Its brightest [G/star] is Gamma Normae [S/243643]. "Must See" objects include: two galactic [G/cluster]s, [N/NGC 6067] and [N/NGC 6087]. The only claim to fame for this [G/constellation] is that it lies in the vicinity of the south [G/celestial pole]. In fact, one of its fainter [G/star]s, Sigma [S/258857], can be considered the South Star. Its brightest star is Nu Octantis [S/257948]. Octans is a [G/circumpolar] constellation and can be seen year round from the southern hemisphere. The legend most often connected with Ophiuchus involves a man named Asclepius, who eventually became the god of medicine. Asclepius once killed a snake that had crawled into his hut. Another snake entered the hut, carrying a strange herb in its mouth. It placed the herb in the mouth of the dead snake. Much to Asclepius' surprise, the first snake came back to life. Asclepius retrieved the strange, life-giving herb from the snake and began using it on humans. The healing power of this herb was great and news of Asclepius traveled quickly. He brought so many people