Catalogues

Aquila / Yale Bright Star Catalog (HR)

«Yale Bright Star Catalogue, 5th Revised Ed.» Hoffleit D., Warren Jr W.H., 1991 [154]
HRBFDMHDSAOFK5IRM*ADSVarIDRADecvMagspTypedMagSepRemarks
HR 70404BD+01 3766173370123879 1129018 44 49.9+02 03 365.02 B9V eS:Shell star. H alpha emission.,VAR:Gamma Cas?, 5.00 - 5.05V.
HR 70595BD-01 355917365414260611667 18 46 28.5-00 57 425.90 A2Vm 1.612.8D:AB binary, B, Am, F3Vm, or Am(A5/F1/F2), RV +9.2k/s, vsini =<25k/s. C, 11.3v optical.,G:Sirius group; UMa stream.,S:Also classified Am(A1/A7V/A7).,SB:ADS 11667A, spectrum binary, RV var.? Unresolved by speckle interferometry on 1976.30; companion with sep. 0.13" seen,SB:on 1980.48 (McAlister and Hartkopf).
HR 7085BD+00 4027174240123947 18 49 37.1+00 50 096.25 A1V
HR 7099BD+10 3685174569104170I11750 18 50 45.6+10 58 356.55 R K5III+K3III 1.13.5D:Binary, companion K3III-IV.
HR 71018BD-03 43921745891427063500 18 51 22.1-03 19 046.10 F2III
HR 7135BD+06 39781755151240503509I 1153618 55 27.5+06 36 555.57 K0III SB:2994d, K 4.65k/s, V0 +23.31k/s, asini 186.
HR 7143BD-01 36021756401428253510 18 56 22.7-01 48 006.22 B9III S:HgMn star.
HR 7163BD+06 3989176095124112 18 58 23.8+06 14 256.21 F5IV
HR 7165BD+17 379917615510429611884 FF Aql18 58 14.7+17 21 395.38 F8Ib 5.36.6D:Companion blue star?,SB:1435d, K 3.5k/s, V0 -17.4k/s, asini 69.1. RV may also vary in 4109d.,VAR:ADS 11884A, CDelta 5.18 - 5.68V, 4.470916d. Magnetic field. Possible blue companion.
HR 716710BD+13 3838176232104303 V1286 Aql18 58 46.9+13 54 245.89 F0pSrEu G:Sirius group?,S:Oxygen deficient relative to magnesium. Magnetic star. Also classified A4p.,VAR:Alpha CV 5.83 - 5.93V. Published periods of 6.05 and 9.78d probably spurious; nor does a more recent 6.5386d satisfy,VAR:all observations. Period may be years. Abt and Golson found range 5.83 - 5.91V. Two isolated obs. of 5.93 and 5.94V,,VAR:while other observers report intermediate values with amp. <0.015V.
HR 717211BD+13 384117630310430811902 1161818 59 05.7+13 37 215.23 F8V 4.317.8D:Both companions optical.,G:UMa stream.
HR 7173BD+09 3951176304104313 18 59 17.5+10 08 276.75 B2Vp
HR 7176ε13BD+14 3736176411104318712IW 18 59 37.4+15 04 064.02 K1-IIICN0.5Ba0.2 5.9131.1C:V magnitudes scatter from 5.56 to 5.81, B-V from +0.35 to +0.45, U-B from -0.01 to +0.04.,N:Deneb el Okab; Deneb. Names combined with HR 7235.
HR 719312BD-05 4840176678142931I 1165519 01 40.8-05 44 204.02 K1III v
HR 7208BD+08 3951176981124184 19 02 21.6+08 22 276.30 K2III
HR 720914BD-03 4460176984142959W 19 02 54.5-03 41 565.42 A1V 0.00.1D:Sep. 0.099". Consistently unresolved by speckle observations at five epochs between 1977.48 and 1981.47 (McAlister,D:and Hartkopf).,G:Hyades group.
HR 7214BD+01 3865177178124203 19 03 32.2+01 49 085.83 A4V
HR 7219BD+03 3882177332124219 19 04 10.7+03 19 506.73 A5m
HR 7220BD-05 4858177336142985I V Aql19 04 24.2-05 41 066.90 C5II VAR:SRb 6.6 - 8.4v, 10.6 - >12.4p, 353d. Mean mag. varies in cycle of about 2270d.
HR 722515BD-04 4684177463142996I12007 A19 04 57.6-04 01 535.42 K1III 1.638.5D:Companion gK4, optical.
HR 7231BD-01 3642177552143003 19 05 18.6-01 30 466.53 F1V
HR 7235ζ17BD+13 3899177724104461716I12026 1172419 05 24.6+13 51 482.99 A0Vn 8.4158.6DYN:0.020".,G:Pleiades group.,N:Deneb el Okab; Deneb. Combined with HR 7176.
HR 7236λ16BD-05 4876177756143021717I 19 06 14.9-04 52 573.44 B9Vn
HR 7243BD+08 3970177940124266IW R Aql19 06 22.2+08 13 486.09 M7IIIe v5.0180.7S:OH and H2O emission. IR spectra show water vapor. OH, H2O and SiO maser. Also classified M5e-M9e.,VAR:M 5.5 - 12.0v, 284.2d. Period changes 348.980 - 0.554202n + 0.000552309n2 from JD 2399190. Radio flare detected,VAR:in this position.
HR 7245BD+00 4106178065124282 19 07 09.1+00 38 306.56 B9III RV:Period 6.87d.,S:HgMn star.
HR 724818BD+10 37871781251044883525 Y Aql19 06 58.6+11 04 175.09 B8III G:Possible Pleiades group.,SB:1.3023d, K 27.6k/s, V0 -18.7k/s, asini 0.494.,VAR:E 5.02 - 5.06B, 1.30227d. Form of light curve possibly variable.
HR 726619BD+05 40401785961243183530 19 08 59.9+06 04 245.22 F0III-IV
HR 7269BD-00 3662178744143087 19 09 51.6-00 25 416.34 B5Vn
HR 727920BD-08 48871794061431341500 1180819 12 40.7-07 56 225.34 B3V
HR 728721BD+02 3824179761124408353712182 V1288 Aql19 13 42.7+02 17 375.15 B8II-III 7.536.2D:Companion optical.,VAR:Alpha CV 5.06 - 5.16V, 1.73d.
HR 7288BD+05 4081179791124410 1182719 13 44.1+05 30 576.49 A2Vp S:Lambda Boo star, Mg 4481 wk.
HR 7300BD+14 3846180262104655W 19 15 20.1+15 05 015.57 G8II-III 2.189.6D:Binary. Companion A1V.
HR 730322BD+04 4045180482124455 19 16 31.0+04 50 055.59 A3IV
HR 7307BD+14 385218055510466812248 19 16 26.8+14 32 415.63 B9.5V 3.88.2D:AB CPM, B is 9.07V, +0.14(B-V), -0.05(U-B), F8V or G0IV, optical? Speckle interferometry indicates a fourth companion,D:at 0.051" from A.
HR 7313BD+01 3960180782124478 19 17 48.2+02 01 546.19 A1Vn S:High velocity metal-rich subgiant.
HR 7315ω125BD+11 3790180868104691725 19 17 49.0+11 35 435.28 F0IV
HR 731923BD+00 4168180972124487I12289 1188919 18 32.5+01 05 075.10 K2II-III v4.13.1D:AB binary. C, 13.7v at 12" optical.,DYN:0.004".
HR 732124BD+00 4170181053124492W 19 18 50.9+00 20 216.41 K0-IIIa:Ba0.4CH1 0.2423.4
HR 7325BD+09 4057181122124497 19 18 52.7+09 37 056.32 G9III G:Wolf 630 group.
HR 733128BD+12 3879181333104722W V1208 Aql19 19 39.3+12 22 295.53 F0III 3.560.2VAR:Delta Sct 5.51 - 5.57V. Period analyses of new and existing data by Reed and Welch (1988, AJ, 95, 1510) indicate a,VAR:possible change in pulsational modes during the last several years, with fundamental period of 0.146d and possible,VAR:nonradial pulsations of 0.141, 0.183, and 0.091d.
HR 7332ω229BD+11 3802181383104728 19 19 53.0+11 32 066.02 A2V
HR 733326BD-05 49361813911432863544IW 19 20 32.9-05 24 575.01 G8III-IV 6.8115.9D:B probably optical.,M:Possible X-ray source 3U1915-05.,SB:266.544d, K 29.9k/s, V0 -18.0k/s, asini 61.1. High orbital eccentricity, 0.83.
HR 733627BD-01 3716181440143292 19 20 35.7-00 53 325.49 B9III
HR 7347BD-08 4950181858143321 19 22 20.7-08 12 046.31 B3IVp
HR 7349BD-00 37251819071433243546 19 22 21.5-00 15 095.83 gG8
HR 7353BD-07 4942182038143340I 19 23 04.6-07 24 016.32 K0
HR 7354BD+09 40811821011245643548 19 22 48.4+09 54 476.35 F6V
HR 7357BD+14 3896182239104779 19 23 08.2+14 55 166.64 F1V
HR 7366BD-05 4964182475143373 19 25 01.6-04 53 036.52 A9V
HR 737331BD+11 38331825721048071503W 1199419 24 58.2+11 56 405.16 G8IVHdel 1 3.5105.6D:Unresolved by speckle interferometry 1986.46.,G:61 Cyg group.
HR 7377δ30BD+02 3879182640124603730IW 1200419 25 29.9+03 06 533.36 F3IV 7.5108.9D:Component A astrometric binary, A* 3.36 F0IV, 3.422y, a = 0.058"; unresolved by speckle interferometry.,SB:0.1571d.,VAR:Delta Sct? Proper motion slightly variable?
HR 7387ν32BD+00 4206182835124628IW 1202119 26 31.1+00 20 194.66 F2Ib 4.2201.0C:V magnitudes scatter from 4.64 to 4.72, B-V from +0.58 to +0.61, U-B from +0.33 to +0.59.,D:Colors of B are +0.31(B-V), +0.16(U-B).
HR 7389BD+12 3907182900104832 19 26 24.1+13 01 265.74 F6III G:Hyades group.,S:Also classified F7IV and F6V.
HR 7396BD+13 40201831441048623555 1204919 27 33.9+14 16 576.32 B4III
HR 7397BD+02 3892183227124661 19 28 20.8+02 55 495.85 B6III
HR 740035BD+01 4010183324124675 19 29 01.0+01 57 015.80 A0IVp G:In Ursa cluster?,S:Lambda Boo star, Mg 4481, met. wk.
HR 7402BD-07 496818334414345412503 U Aql19 29 21.5-07 02 386.61 F7-G1I-II v5.51.5D:AB fixed. C, 7v at 2", binary.,S:Also classified F5I-II-G1.,VAR:ADS 12503A, CDelta 6.08 - 6.86V, 7.02393d. Period changes.
HR 7404BD-00 3760183387124681I 19 29 18.0+00 14 466.25 K2
HR 7407BD+14 3936183492104896 19 29 22.1+14 35 455.56 K0III
HR 7412BD+02 3904183589124698I12520 1208819 30 10.5+02 54 156.09 K5Ib 4.934.1D:B, optical.
HR 741436BD-03 46121836301434821509I 1209319 30 39.8-02 47 205.03 M1III v
HR 7415BD+03 4043183656124704 V923 Aql19 30 33.1+03 26 406.05 A0eShell S:He lines widened by rotation; NaI lines narrow. Also classified B9.5Ia. Line profiles vary.,VAR:Gamma Cas, amp. 0.12V, 0.8518d. Variation may be due to rotation and inhomogeneous distribution of brightness on disk.
HR 7429μ38BD+07 41321844061247991511I12607 1215519 34 05.4+07 22 444.45 K3-IIIbCN0.5 5.0177.5D:B and C optical.
HR 743037BD-10 51221844921627923562I 19 35 07.3-10 33 375.12 G9IIIa
HR 7432BD-07 4998184573143564 19 35 29.8-07 27 376.34 K0
HR 7438BD+02 3932184663124823 19 35 25.2+02 54 486.38 F6IV
HR 7445BD+10 398118488410503212660 19 36 08.0+11 09 006.68 A3V 6.43.8
HR 7446κ39BD-07 5006184915143600737I 1220419 36 53.5-07 01 394.95 B0.5III G:Sct OB2.
HR 7447ι41BD-01 378218493014359712663 1220119 36 43.3-01 17 114.36 B5III 8.947.0G:Member of the local association (Pleiades group).
HR 7449BD+14 3974184944105036 19 36 15.8+14 23 306.38 K0II-III
HR 7456BD+10 398418501810504512670 19 36 52.5+11 16 245.98 G0Ib 5.780.
HR 746042BD-04 4861185124143621 19 37 47.3-04 38 515.46 F3IV
HR 7471BD+03 40971854231248923569 19 38 49.0+03 22 546.35 B3III
HR 7474σ44BD+05 422518550712490312737 Sig Aql19 39 11.6+05 23 525.17 B3V+B3V v6.647.8D:B, 12v K0Ve at 48" optical. C, 12v at 130". Rotational velocity of A 123k/s, of B 142k/s.,SB:ADS 12737A, 1.950271d, K 164.2k/s, V0 -4.5k/s, msin3i 5.84, asini 4.40. vsini of secondary 129k/s.,VAR:ADS 12737A, EB 5.18 - 5.36B, 1.95026827d. i 71.7d. Spectra vary in period 1.950271d.
HR 748045BD-00 3813185762143678357312775 19 40 43.3-00 37 165.67 A3IV 7.242.0D:A companion at 0.084" discovered by speckle interferometry.
HR 7486BD+13 40981859361051323574W QS Aql19 41 05.5+13 48 566.01 B5V 0.20.1D:Speckle interferometry 1985.5 gives sep. 0.178".,G:Member of the local association (Pleiades group).,SB:2.4968d, K 47.3k/s, V0 -14.2k/s, asini 1.62. Equal components.,VAR:Primary of visual double, EA 5.93 - 6.05V, 2.513294d. Double unresolved in 1961 when period changed sharply.
HR 749346BD+11 3954186122105156 19 42 12.8+12 11 366.34 B9IIIpHgMn
HR 7497χ47BD+11 395518620310516812808 1232519 42 34.0+11 49 365.27 G0:III+A3V 1.20.4D:AB, fixed sep.,DYN:0.0006".,S:Also classified G2+B8 and dF3+A3.
HR 7511ψ48BD+12 4059186547105199 19 44 34.1+13 18 106.26 B9III-IV SB:Double lines suspected.
HR 7516BD-03 47011866601437763579 19 45 52.2-02 53 006.48 B3III
HR 7519υ49BD+07 4210186689125032 19 45 39.9+07 36 485.91 A3IV
HR 7525γ50BD+10 4043186791105223741IW 19 46 15.6+10 36 482.72 K3II e8.0132.6N:TARAZED; Reda.,S:Ultraviolet FeII emission.
HR 7541BD-11 5131187195163012 19 49 02.2-10 52 156.04 K5III
HR 7542BD+10 4058187203105278 19 48 30.4+10 41 396.44 F8Ib-II
HR 7544π52BD+11 399418725910528212962 1242519 48 42.1+11 48 575.72 G2III:+A1V: 0.51.4D:AB, >3000y.
HR 755351BD-11 514918753216303674413017 19 50 46.8-10 45 495.39 F0V 8.021.1D:Optical.
HR 7554BD+07 4252187567125116S V1339 Aql19 50 17.5+07 54 096.51 B2.5IVe 0.1VAR:Gamma Cas? 6.33 - 6.52V.
HR 7557α53BD+08 4236187642125122745I13009 19 50 47.0+08 52 060.77 A7V 8.6165.2D:Component B optical.,N:ALTAIR; Atair.,R:Diam. = 0.00278 - 0.00298".
HR 7559BD-02 5133187660143853I 19 51 11.1-02 27 396.13 K5III
HR 7560ο54BD+10 407318769110533813012 19 51 01.6+10 24 565.11 F8V 8.314.4D:Component B optical. AC, 13.8 dM4, 22" binary.
HR 7562BD+09 4288187753125139 19 51 17.7+09 37 496.25 A1m
HR 7569BD+11 4019187923105348W 1249019 52 03.5+11 37 446.13 G0V 5.590.5
HR 7570η55BD+00 4337187929125159746I Eta Aql19 52 28.4+01 00 203.90 F6Ib vS:Also classified F6Ib-G4Ib. UV suggests A0V companion.,VAR:Discovered by Pigott in 1784. CDelta 3.50 - 4.30V, 7.176641d. Period changes. Variable He 10830 in emission and,VAR:absorption.
HR 7572BD+09 429518796110535513041 1249619 52 15.6+10 21 056.54 B7V 4.013.5D:Component B = A3V.,G:Member of the local association (Pleiades group).
HR 7575BD-03 47421880411438831519 V1291 Aql19 53 18.7-03 06 525.65 A5p vS:Also classified F0p SrCrEu.,VAR:Alpha CV 5.61 - 5.67V, 224.5d. Also period for spectrum and magnetic field var. Rotation 226d.
HR 7580BD+04 4264188107125182 19 53 22.6+04 24 026.53 B9.5Vn
HR 758456BD-08 5150188154143894IW 19 54 08.2-08 34 275.79 gK5 6.146.5
HR 759357BD-08 515418829314389813087 A19 54 37.6-08 13 385.71 B7Vn 0.835.7D:CPM with HR 7594.
HR 759457BD-08 515518829414389913087 B19 54 38.1-08 14 146.49 B8V 0.835.7D:CPM with HR 7593.
HR 7595ξ59BD+08 4261188310125210I 19 54 14.9+08 27 414.71 G9+IIIb
HR 759658BD-00 3871188350125219 19 54 44.8+00 16 255.61 A0III
HR 7598BD+06 435118838512522113093 19 54 40.3+07 08 256.15 A2V 6.413.8D:Optical.
HR 7599BD-07 510218840514391113104 19 55 19.6-06 44 036.51 F2V 1.10.2D:Speckle interferometry 1985.5 gives sep. 0.173".
HR 7602β60BD+06 4357188512125235749I13110 1255719 55 18.8+06 24 243.71 G8IV 7.7175.0D:AB binary. B 12v dM3 at 13".,DYN:0.049".,N:ALSHAIN; Alschairn.,VAR:ADS 13110A, amp. 0.05V.
HR 7610φ61BD+11 40551887281054383590 19 56 14.3+11 25 265.28 A1IV SB:3.3207d, K 37.2k/s, V0 -28.0k/s, asini 1.70.
HR 7636BD+00 43751893221253103596 19 59 22.7+01 22 406.17 G8III
HR 7637BD-10 5238189340163168W 19 59 47.4-09 57 305.88 F8V 0.00.1
HR 7648BD+08 4300189695125355I 20 00 58.9+08 33 295.91 K5III
HR 7661BD-07 5159190172144038 20 04 01.2-07 28 116.72 F4III
HR 7664BD+15 4033190229105615 20 03 30.0+16 01 535.67 B9pHgMn G:Member of the local association (Pleiades group).,N:14 Sge, in Aquila.,RV:61.7d? Earlier vsini 61k/s.
HR 766762BD-01 3887190299144045I 20 04 23.2-00 42 345.68 K4III
HR 7669τ63BD+06 44161903271254031524I 20 04 08.3+07 16 415.52 gK0
HR 7671BD-12 5641190390163245W V1401 Aql20 05 05.4-11 35 586.34 F1III 25. D:Discovered as double by W. Herschel; companion not rediscovered.,S:Probably a supergiant.,VAR:SRd 6.18 - 6.55V, 28.49d.
HR 7680BD+15 4040190658105663I13344 20 05 26.5+15 30 016.34 M2.5III 4.02.7D:CPM.
HR 7681BD-04 5013190664144062 20 06 12.2-04 04 426.47 K0
HR 769064BD-01 3899191067144095 20 08 01.8-00 40 425.99 K1IV
HR 7693BD+08 434419110412547813403 20 07 50.3+09 23 596.43 F3V 2.13.1D:Binary.
HR 7700BD+10 41891912631057433616 20 08 38.3+10 43 336.31 B3V G:Member of the local association (Pleiades group).
HR 7710θ65BD-01 3911191692144150756IW 20 11 18.3-00 49 173.23 B9.5III 9.6113.7G:In reflection nebula.,SB:17.1243d, K 51.0k/s, V0 -27.9k/s, msin3i 0.742, asini 9.52.
HR 7717BD+00 444419198412556713506 A20 12 35.2+00 52 036.27 B9pCrEu:Sr: 0.22.8D:Discordance as to which component has the peculiar spectrum usually attributed to A. However, on the basis of better,D:spectrograms, Abt gives A = A0V, B = A0Vp(Sr,Cr st.,Ca wk.).
HR 772066BD-01 3920192107144181I 20 13 13.9-01 00 345.47 K5III S:Very bright in ultraviolet.
HR 7724ρ67BD+14 42271924251058781526 20 14 16.6+15 11 514.95 A2V
HR 7768BD-01 3951193329144296 20 19 43.3-01 04 436.06 K0
HR 7772BD-06 54511934291443133628I 1301320 20 26.1-06 21 426.63 K5 VAR:Amp. 0.06V.
HR 7794BD+04 44341940131257471531 20 23 10.7+05 20 355.31 G8III-IV
HR 7803BD+00 449519424412576913811 1306420 24 37.5+01 04 076.15 B9V 4.731.3D:Discordances as to which component is B, which C. IDS gives B, 13.1v at 17.1".
HR 7809BD-03 4888194454144412 20 25 42.5-02 48 016.11 gK1
HR 782168BD-03 4906194939144468W 20 28 24.9-03 21 286.13 B9V 7.79.8
HR 783169BD-03 49181951351444951533I 20 29 39.0-02 53 084.91 K2III
HR 787370BD-03 49611963211446243648I 20 36 43.6-02 33 004.89 K5II
HR 7878BD-00 4056196426144632 20 37 18.3+00 05 496.22 B8IIIp
HR 788471BD-01 4016196574144649I14081 1318720 38 20.3-01 06 194.32 G7.5IIIa 7.532.2D:Optical.,SB:ADS 14081A, 205.2d, K 9.8k/s, V0 -5.9k/s, asini 27.7.

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