Catalogues

Ara / Yale Bright Star Catalog (HR)

«Yale Bright Star Catalogue, 5th Revised Ed.» Hoffleit D., Warren Jr W.H., 1991 [154]
HRBFDMHDSAOFK5IRM*ADSVarIDRADecvMagspTypedMagSepRemarks
HR 6167CP-60 6594149485253638 16 38 52.7-60 59 256.18 B7Vn
HR 6177CP-60 6603149837253651W 16 40 50.5-60 26 466.18 F2III-IV 2.71.4
HR 6187CD-4811070150136227049W A16 41 20.3-48 45 475.65 O5III(f) 1.29.6D:AB binary, 5.6, 9.0v sep. 1.6". C = HD 150135, O7:, CPM.,G:In cluster NGC 6193 #1. Neutral hydrogen shell around the cluster probably at greater distance and not associated with,G:the cluster. High luminosity member of Ara OB1a complex.,S:Also classified O5III:n(f).,SB:Component A of visual system.
HR 6188CD-49108901501682270583321 16 41 40.2-49 39 065.65 B1Iab-Ib G:Ara OB1a; in HII region.
HR 6197CD-4510858150421227092 16 43 03.4-46 04 146.23 F5Iab G:Ara OB1.
HR 6207CP-52101611505762441063327W 16 44 39.8-53 09 095.96 G8III 6.040.
HR 6215CP-58 6889150745244122 16 46 21.2-58 30 135.74 B2IV-V
HR 6219CP-58 6893150898244133 16 47 19.5-58 20 295.58 B0.5Ia G:Listed by Buscombe and Kennedy (M.N.R.A.S. 124, 196, 1962) as among Sco-Cen stars. Buscombe now points out that it is,G:a nonmember background star.
HR 6229ηCP-58 69061512492441681435W 16 49 47.1-59 02 293.76 K5III 9.523.6
HR 6236CD-4910998151566227281W 16 50 35.9-50 02 446.47 A5III+F7III 0.13.2D:Secondary = GC 22634, 6.47V A8m. Primary, fast rotation, not Am.,S:Also classified F0IV + F2IV. Primary also classified A8V:n.
HR 6251CP-57 8157151967244245 16 54 00.5-57 54 345.94 M1III
HR 6253CP-63 4032152082253734W 16 55 24.7-63 16 116.02 A0III 6.97. S:Moderately strong shell absorption.
HR 6274CD-5010905152478244280 8047 16 56 08.9-50 40 306.33 B3Vnep S:Shell star.,VAR:Amp. 0.04V. Time scale of 1d suspected.
HR 6275CP-5210333152527244285 16 56 28.7-52 17 025.94 B9V
HR 6285ζCP-55 7766152786244315631 16 58 37.2-55 59 253.13 K3III
HR 6289CD-50109241528242443131444 16 58 18.0-50 38 285.55 B9IV
HR 6295ε1CP-5210372152980244331632 16 59 35.1-53 09 384.06 K4IIIab
HR 6297CP-54 7947153053244338W 17 00 06.2-54 35 495.65 A5IV-V 6.120.1
HR 6300CD-4811360153221227542W 17 00 27.1-48 38 526.00 G8-K0III+G 1.11.0
HR 6304CP-58 6964153261244362 V828 Ara17 01 47.4-58 57 306.11 B2IVne vS:Line width of H alpha varies.,VAR:Gamma Cas 6.11 - 6.20V, time scale 1d suspected.
HR 6312CD-5010955153370244370W 17 01 46.1-51 07 516.45 A7V 0.30.1D:A8, F3, sep. 0.107".
HR 6314ε2CP-53 8316153580244388W 17 03 08.8-53 14 135.29 F6V 7.625.
HR 6320CP-57 82651537162444013355 17 04 24.7-57 42 445.73 B5IV eG:Sco-Cen cluster; member of the local association (Pleiades group); Sco-Cen assoc.,S:Possible H alpha emission.
HR 6323CD-4611191153791227588W 17 03 41.7-47 09 366.06 A2-3V 6.06.2S:Also classified A7V:.
HR 6356CP-61 58421545552538183362 17 10 06.3-61 40 326.39 B8II-III
HR 6368CP-67 3296154903253827W 17 13 17.5-67 11 485.89 K0-1III 3.234.1D:Optical.
HR 6374CD-4811492155035227699 17 11 38.9-48 52 275.84 M1-2III
HR 6384CP-56 8098155341244539 V829 Ara17 14 13.2-56 53 186.09 M1-2II-III+A VAR:Ellipsoidal binary, 6.118 - 6.195V, 80d orbital period.
HR 6408CP-59 6954156091244613W 17 19 12.4-59 41 405.91 K2IIICNIb-II 7.020.
HR 6416CD-4611370156274227816W 17 19 03.2-46 38 025.48 G8-K0V 3.17.5D:AB 5.53 G8V, 8.65 M0V, 693.24y, a = 10.415", or 2205y, a = 23.90". Various published orbits range from 242 to 2205y.,D:Combined mag., colors.,DYN:0.117".,RV:Comp. B, +21k/s.
HR 6423CD-4911324156331244631W 17 19 30.3-50 03 486.27 F8III+B9V 0.00.1D:Sep. 0.108".,S:Also classified F3IV-V.
HR 6438CP-57 8478156768244678W 17 22 55.0-58 00 375.88 G8Ib-II 3.62.0
HR 6440CP-62 55581568382539033378 17 24 01.1-62 51 515.70 B2IV G:Sco-Cen assoc.; doubtful member of the Sco-Cen cluster.
HR 6442CP-56 8191156854244685 17 23 06.9-56 31 315.80 G8-K0III
HR 6447CP-60 6800156942253908 17 24 18.7-60 40 255.77 B8Ib-II
HR 6451ιCD-47114841570422278863379W Iot Ara17 23 16.1-47 28 065.25 B2IIIne v5.342.8D:Companion G5III, optical.,S:H alpha profile varies.,VAR:Gamma Cas? 5.22 - 5.25V on time scale of fraction of a day.
HR 6461βCP-55 8100157244244725645I 17 25 18.0-55 31 482.85 K3Ib-IIa D:Possibly CPM and same RV as HR 6462, 50'N.
HR 6462γCP-56 8225157246244726W 17 25 23.6-56 22 393.34 B1Ib 7.017.9C:Color excess E(B-V) = +0.08.,D:Component B, A7V; C is optical.,G:Sco-Cen assoc.; doubtful member of the Sco-Cen cluster.,S:Unusually large line broadening for luminosity Ib. Also classified B1III.
HR 6468κCD-5011269157457244734W 17 26 00.0-50 38 015.23 G8III 8.330.
HR 6471CP-62 5590157524253928 17 28 07.7-63 02 116.24 B7-8V
HR 6475CD-5110881157599244749 17 26 56.3-51 56 576.19 B8-9V
HR 6477CD-4511531157661227971W 8637 17 26 51.5-45 50 375.29 B7V+B9.5V 0.82.3D:AB binary. Combined mag., colors. Component C, 7.6v at 103".
HR 6478CD-5011283157662244755W 17 27 12.4-50 37 495.92 B9II 4.776.1
HR 6483CP-52106621577532447633386W 17 27 57.6-52 17 505.75 K2III 7.217.
HR 6487CP-55 8144157819244770W 17 28 38.7-55 10 115.94 G8II-III 6.537.0D:B, 14.0v at 15"; C, 12.5 at 37".
HR 6500δCP-60 6842158094253945648W 17 31 05.9-60 41 023.62 B8Vn 8.047.4D:Companion K0III, optical.,G:Pleiades group.
HR 6505CP-56 8304158220244808 17 31 23.0-56 55 145.95 B7II-III
HR 6510αCD-4911511158427228069651W 8999 17 31 50.5-49 52 342.95 B2Vne v8.055.6D:Companion K0IV, optical.,G:Cas-Tau group; member of the local association (Pleiades group); Sco-Cen assoc.; probable member of Sco-Cen cluster.,S:Shell star with variable H alpha emission.,VAR:2.76 - 2.90V.
HR 6513CD-4511626158476228075W 17 31 49.1-46 02 116.03 F8-G0Ib 4.218.0
HR 6525CP-59 7071158895244866 17 35 34.9-59 50 466.28 B5II-III
HR 6530CP-53 8682159018244870 17 35 20.0-53 21 106.10 B9III
HR 6537σ1CD-4611661159217228162 17 35 39.6-46 30 204.59 A0V
HR 6547CD-4911577159463244894 17 37 27.2-50 03 365.93 K0III
HR 6549πCP-54 8403159492244896 17 38 05.6-54 30 015.25 A5IV-V
HR 6569λCD-4911616160032228257 Var?17 40 23.6-49 24 564.77 F3IV VAR:Delta Sct?
HR 6572CD-46117471602632282793404 17 41 16.3-46 55 195.79 A0V
HR 6576CD-5011474160342244954 V626 Ara17 42 03.9-50 30 386.24 M3+II-III VAR:Lb 6.2 - 6.57V.
HR 6585μCD-5111094160691244981662 17 44 08.7-51 50 035.15 G3IV-V
HR 6614CP-55 83121614202450443412 17 48 38.1-55 24 066.11 A9IV
HR 6622CP-53 8799161783245065W V539 Ara17 50 28.2-53 36 445.92 B2V+B3V 3.012.3N:Sometimes called Upsilon1 Ara, more often Nu1; generally no letter.,SB:3.170d, K 154k/s, V0 -6k/s, msin3i 6.67, asini 6.71. Equal components. vsini secondary 119k/s.,VAR:EA 5.66 - 6.18V, 3.169128d.
HR 6632CP-53 8812161917245072 17 51 11.0-53 07 506.09 B9.5III-IV N:Sometimes called Upsilon2, more often Nu2 Ara; generally no letter.
HR 6640CD-4511958162123228490 17 51 44.5-45 36 026.11 G6III
HR 6743θCD-50117201650242452421471 18 06 37.9-50 05 303.66 B2Ib G:Listed by Buscombe and Morris (M.N.R.A.S. 121, 268, 1960) and by Buscombe and Kennedy (M.N.R.A.S. 124, 196, 1962) among,G:Sco-Cen stars. Buscombe now rejects membership, while Eggen (ApJ, 188, 59, 1974) includes it as a member of the,G:Pleiades group.
HR 6759CD-4512215165493228734W 18 08 30.1-45 46 026.15 B7-8II 3.64.0D:Component B, B9V, optical?

Legend

Key to columns [154]
HRHarvard Revised Number = Bright Star Number
BBayer designation (greek letter)
FFlamsteed number
DMDurchmusterung Identification (BD = Bonn; CD = Cordoba; CP = Cape Photographic)
HDHenry Draper Catalog Number
SAOSAO Catalog Number
FK5FK5 star Number
IRI if infrared source
M*Double or multiple-star code. (A = Astrometric binary; D = Duplicity discovered by occultation; I = Innes, Southern Double Star Catalogue (1927); R = Rossiter, Michigan Publ. 9, 1955; S = Duplicity discovered by speckle interferometry; W = Worley (1978) update of the IDS;)
ADSAitken's Double Star Catalog (ADS) designation
VarIDVariable star identification
RARight Ascension (J2000.0)
DecDeclination (J2000.0)
vMagVisual magnitude
spTypeSpectral type
dMagMagnitude difference of double, or brightest multiple
SepSeparation of components in Dmag if occultation binary (arcsec)
RemarksNote on Category (C = Colors; D = Double and multiple stars; DYN = Dynamical parallaxes; G = Group membership; M = Miscellaneous; N = Star names; P = Polarization; R = Stellar radii or diameters; RV = Radial and/or rotational velocities; S = Spectra; SB = Spectroscopic binaries; VAR = Variability)

References