Kataloge

Sagittarius / Yale Bright Star Catalog (HR)

«Yale Bright Star Catalogue, 5th Revised Ed.» Hoffleit D., Warren Jr W.H., 1991 [154]
HRBFDMHDSAOFK5IRM*ADSVarIDRADecvMagspTypedMagSepRemarks
HR 66163CD-27119301615921857551464I X Sgr17 47 33.6-27 49 514.54 F7II VAR:CDelta 4.24 - 4.84V, 7.01225d.
HR 6617BD-22 4423161664185765I 9682 17 47 45.6-22 28 416.18 G6IbHdel 1
HR 6621CD-2612367161756185779 V3894 Sgr17 48 27.8-26 58 306.35 B4IVe G:Sco-Cen assoc.,VAR:6.27 - 6.39V. Amp. 0.05V on time scale 3 hrs and 0.08 on time scale 1d suspected.
HR 6672CD-2413615162978185928 17 54 54.0-24 53 146.20 O7.5II((f)) G:Within 0.5d of HII reg. Ma 336.,S:Also classified O8III, O8IIIf, O8.5III((f)), O8II(f) O7.5II((f)) and O9.5Ib. uv 1394 and 1548 absorption very strong;,S:1548 emission weak.
HR 6679BD-18 46861632451609093423 17 55 55.0-18 48 086.52 A4V G:In cluster NGC 6494 #1.
HR 6680CD-2813878163318185975 17 56 41.9-28 03 555.80 A7III/V:
HR 6691CD-3612060163652209545W 17 58 55.6-36 51 305.74 G8III 2.451.7D:Companion F0.
HR 6692CD-2813936163685186025D 17 58 39.1-28 45 336.01 B3IV 1.00.3D:Doubtful double, 6.3, 7.3v, sep. 0.3".
HR 6693CD-30150351637550IW A9929 17 59 05.2-30 15 115.16 M1Ib 1.85.5C:V magnitudes scatter from 4.98 to 5.14, B-V from +1.62 to +1.76, U-B from +1.52 to +1.93.,D:Fixed with HR 6694. Mag. and colors combined light, 4.98V, +1.63(B-V), +1.52(U-B).,VAR:4.96 - 5.00V for combined light with 6694. Uncertain which varies, probably 6693.
HR 6694CD-3015035163756209553W B9929 17 59 05.5-30 15 127.04 G8II 1.85.5D:Fixed with HR 6693.
HR 67004CD-23137311639551860613430 17 59 47.6-23 48 584.76 B9V
HR 6704BD-20 4940164028186070D 18 00 00.1-20 20 216.21 K0II-III D:Suspected occultation double.
HR 6708CD-3612115164245209608 18 01 48.3-36 22 406.30 B7IV
HR 67156BD-17 49871643581609981470I 18 01 23.1-17 09 256.28 K3III
HR 6716BD-22 4503164402186135I10983 9996 18 01 54.4-22 46 505.77 B0Ib 7.18.2C:May not be the IR source. Strong IR excess probably due to circumstellar dust envelope. Color excess E(B-V) = +0.37.,G:Sgr OB1; in cluster M20.,S:Nitrogen deficient.
HR 67247CD-2413793164584186163 18 02 51.1-24 16 565.34 F3III G:NGC 6530 #4.
HR 6727BD-22 4516164637186169 18 03 01.7-22 43 066.74 B0.5III G:Sgr OB1.
HR 67369CD-2413814164794186204I 18 03 52.4-24 21 385.97 O4V((f)) C:Color excess E(B-V) = +0.34.,G:Cluster NGC 6530 #7; Sgr OB1; in HII reg. S25; in nebulosity.,S:uv observations indicate dwarf; 1548 emission very strong.
HR 6739CD-35122291648702096713435W 18 04 50.4-35 54 056.00 K2III 5.212.5
HR 6742γ1CD-291444716497518623711029 W Sgr18 05 01.3-29 34 484.69 F4-G1Ib v0.00.1D:ADS 11029A is speckle interferometric double, sep. 0.116". Visual companions, 13.5v at 33" and 13.5v at 48".,N:Although HR 6742 and 6746 are named gamma1 and gamma2 Sgr, respectively, more often 6746 is simply called gamma Sgr,N:and the Greek letter is omitted for HR 6742.,SB:80y, K 2.65k/s, V0 -27.7k/s, asini 60.,VAR:ADS 11029A, CDelta 4.30 - 5.08V, 7.594710d. Period changes. Spectrum and magnetic field variable. One component of,VAR:SB.
HR 6746γ210CD-3015215165135209696679I 1017318 05 48.5-30 25 272.99 K0III G:Wolf 630 group.,N:Nash; Alnasl; Alwazl; Zujj al Nushshabah; Nushaba. Gamma1 or gamma2 Sgr; see HR 6742.
HR 6748CD-3612214165185209710 18 06 23.7-36 01 115.95 G5V
HR 6762BD-21 48551655161863023438 18 07 11.4-21 26 386.28 B0.5Ib G:Sgr OB1; in HII region.
HR 6766CD-28141741656341863283439ID 18 08 05.0-28 27 264.57 G7:IIIb* 0.80.3D:5.1, 5.9, sep. 0.26", doubtful duplicity.,S:G7:IIIb CN-1 CH-3.5 HK1. Also classified G8IIIp CH-3 CN-2. Weak G-band.
HR 6769BD-17 5028165687161093I 18 07 48.4-17 09 155.52 K1III
HR 6772CD-3612265165793209779 18 09 22.4-36 40 216.58 B1II
HR 6773CD-2512793165814186350W V3792 Sgr18 08 54.1-25 28 216.61 B3III 2.013.3D:Visual companion is blue.,SB:2.2481d, K 151k/s, V0 -6k/s, msin3i 6.42, asini 4.66. Mean mass components 5.5 solar.,VAR:EB 6.43 - 6.88V, 2.24815d. Mass transfer indicated. The var. is probably the 8.85V companion of the visual double. GCVS,VAR:gives combined light.
HR 6777CD-3213814165978209794 18 09 59.9-32 43 116.43 K0IV
HR 6780CD-3015316166023209803W 18 10 05.7-30 43 435.53 K1II 2.33.9D:Binary. Combined mag., colors. Component B is F0IV or F0V.,RV:Comp. B, -17k/s.,S:Also classified K0IIIab.
HR 6788CD-3312917166197209817 1030418 10 55.2-33 47 596.16 B1V
HR 6798BD-19 488616639316115311127 18 11 14.8-19 50 326.36 A4V 0.41.2D:AB visual double, A4V, F0, combined mag., color. Third component found by lunar occultation, 1.3B, 0.9R fainter than B,,D:sep. 0.024".
HR 680111CD-2314047166464186437I11133 18 11 43.4-23 42 044.98 K0III 5.742.1D:Companion, 11.52V, +0.66(B-V), +0.11(U-B), F8V:
HR 6802CD-2814268166469186444 V4045 Sgr18 11 58.2-28 54 056.51 B9IVpSrEuCr VAR:Amp. 0.013v, 2.8855d.
HR 6812μ13BD-21 490816693718649768211169 Mu Sgr18 13 45.8-21 03 323.86 B8Iap e2.90.0D: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:D, 9.9v, B3; E, 9.4v, B2V, physical, vsini 184k/s.,G:Sgr OB1.,S:Shell star.,SB:ADS 11169A, 180.45d, K 56.8k/s, V0 -2.7k/s, asini 129.,VAR:ADS 11169A, EA 3.79 - 3.92V, 180.45d. Also irregular changes in brightness.
HR 681614BD-21 4916167036186509I 1039318 14 15.9-21 42 475.44 K3III S:Case infrared spectra indicate M3.
HR 682215BD-20 5054167264186543 18 15 12.9-20 43 425.38 B0Ia G:Sgr OB7; exciting star of HII region S35; NGC 6526. Also classified O9.7Iab.
HR 682316BD-20 505516726318654411191 18 15 12.9-20 23 175.95 O9.5II v7.06.0D:Companion A3V.,G:Sgr OB7; exciting star of HII region S35; NGC 6526.,S:SiII suspected of variability. Also classified O9II, O9III and O9.5II-III((n)).
HR 6825BD-18 486416735616122711196 18 15 30.8-18 39 416.07 A0Ia 5.710.1D:Double may be spurious: companion not seen in 1934.,G:Sco-Cen assoc.
HR 6832ηCD-3612423167618209957683IW Eta Sgr18 17 37.6-36 45 423.11 M3.5III e4.93.5S:Ultraviolet FeII emission.,VAR:Lb 3.08 - 3.12V.
HR 6833CD-3412673167647209959W RS Sgr18 17 36.1-34 06 266.16 B3V+A 2.694.1D:B, 9.68V at 39"; CD, 8.7, 10.2v, sep. 16.5".,S:Also classified B4IV.,SB:2.4157d, K 85.1k/s, V0 +6.0k/s, asini 2.82.,VAR:EA 6.0 - 6.9p, 2.4156832d. Period changes. Component A of visual double.
HR 6835CD-2814407167666186594 18 17 24.0-28 39 096.19 A5/7V
HR 6836CD-2814408167665186593 18 17 23.7-28 17 216.40 G0V
HR 6838BD-17 51121677201612603454I 18 17 11.6-17 22 265.75 K4II-III
HR 6841BD-18 4886167771161267W 18 17 28.5-18 27 486.54 O7III:(n)((f)) 6.68.4D:Companion A3V, optical?,G:Sgr OB4; exciting star of HII region S41; within 0.5d of S39.,S:Also classified O7If and O8I(f).,SB:3.9735d, K1 107.1k/s, K2 122.9k/s, V0 +9.1k/s, m1sin3i 2.7, m2sin3i 2.3, a1sini 5.8,,SB:a2sini 6.7.
HR 6842CD-2712684167818186612I 18 18 03.2-27 02 334.65 K3II
HR 6846CD-2512995167979186629I 18 18 41.7-25 36 176.51 gK1
HR 6848BD-18 489616802116130411240 1054318 18 43.3-18 37 106.84 B0Ib 0.50.4D:AB binary. C, 8.0v B0.5Ib at 18", vsini 42k/s.,G:Sgr OB4; exciting star of HII region S41; within 0.5d of S39.
HR 6859δ19CD-2914834168454186681687I11264 18 20 59.7-29 49 412.70 K3-IIIa* 10.258.1N:Kaus Meridionalis; Kaus Media; Media.,S:K3-IIIa CN0.5 Ba0.2 Fe0.5. Also classified K3IIIa CN 1 Ba 0.1 Fe 0.5.
HR 6861CD-2414219168574186699I V4028 Sgr18 21 31.4-24 54 546.25 M5III R:Occult diam. = 0.0032".
HR 6863BD-18 4926168608161376 Y Sgr18 21 23.1-18 51 365.75 F8I RV:Possibly long period.,VAR:CDelta 5.40 - 6.10V, 5.77335d.
HR 6864CD-2814495168646186704 18 22 00.2-28 25 486.16 A3III S:Strong shell absorption; no emission.
HR 6870CD-3612524168733210061 V4050 Sgr18 22 53.1-36 40 105.34 Ap G:Member of Pleiades group.,S:Chlorine in spectrum. Iron-rich star with overabundant titanium and chromium.,SB:11.7d. K =<0.5k/s.,VAR:Amp. 0.01v, 6.3d. Weak variable magnetic field, 14.6d.
HR 6874CD-3612537168838210075 18 23 28.9-36 14 185.55 K0III
HR 6879ε20CD-3412784169022210091689W 18 24 10.3-34 23 051.85 B9.5III 12.336.1N:KAUS AUSTRALIS.,R:Diam. = 0.00137 - 0.00144".,RV:Two discordant determinations of vsini, 0 and 175k/s.
HR 688818CD-3015661169233210116I 18 25 01.5-30 45 245.60 K0III-IV
HR 6889CD-3612589169236210119 18 25 21.7-35 59 306.15 K0III
HR 6893CD-3412802169398210135 18 25 54.6-33 56 436.30 B5IV
HR 689621BD-20 5134169420186794I11325 18 25 21.0-20 32 304.81 K2II 3.61.7D:Companion is A5:.,DYN:0.006".,G:Red star Pleiades group.
HR 6907CD-2914965169830186838 18 27 49.5-29 48 595.92 F9V
HR 6909CD-261318416985118683711354 18 27 43.8-26 38 056.31 A8V+F2V 0.01.1D:Combined spectrum A5; component B, A8V:.
HR 6913λ22CD-2513149169916186841692I 18 27 58.2-25 25 182.81 K1+IIIb G:Hyades group.,N:Kaus Borealis.,R:Occult diam. = 0.0044".
HR 6914CD-2613192169938186843 18 28 06.2-26 45 266.27 A3/4V
HR 6919BD-17 5203169990161493I 1083518 27 56.5-17 48 006.20 B8V
HR 6926CD-2613206170141186863W 1086418 28 57.4-26 34 546.50 A3III 1.741.9VAR:Amp. 0.24V.
HR 6929CD-2513170170235186873 V4031 Sgr18 29 22.0-25 15 236.59 B2IVpe vS:Shell star.,VAR:Amp. 0.10V. Spectrum (Balmer emission lines) variable.
HR 6933BD-18 4982170433161540 18 30 11.9-18 43 445.66 gK0
HR 6936CD-3313281170479210257W 18 31 04.8-32 59 215.34 A3m 4.53.4D:AB, CPM.,S:Also classified A3m.
HR 6944BD-18 498817068016156411411 18 31 26.3-18 24 105.14 A0Vp 8.925.2D:Binary.,G:Hyades group.,S:Lambda Boo star, Ca, Mg 4481 wk.
HR 6947BD-19 5047170764161571W U Sgr18 31 53.3-19 07 306.68 G1.5Ib 2.0430.7G:M25; in cluster IC 4725 #103.,VAR:CDelta 6.34 - 7.08V, 6.744925d. May have blue companion.
HR 6960CD-33133381710342103123471 18 33 57.8-33 01 005.28 B2IV-V G:Sco-Cen assoc.
HR 696124CD-2414472171115186981I 18 33 53.5-24 01 575.49 K4Ib
HR 696525CD-2414479171237186995 1103518 34 32.8-24 13 216.51 F3II-III VAR:Delta Sct?
HR 6969BD-20 5189171369187012 18 35 21.3-20 50 276.48 F0IV
HR 6972CD-29151231714161870243478 18 35 59.7-29 41 576.37 K1III
HR 6988BD-21 50761718561870711485D 18 37 54.4-21 23 525.94 A8IIIn 0.00.1D:Possible binary listed by D. W. Dunham, 6.5, 6.5, sep. 0.1".
HR 6990CD-2314572171961187080 18 38 30.7-23 30 185.81 B8III SB:Double lines suspected.
HR 6998BD-21 5081172051187086 18 38 53.4-21 03 075.86 G4V
HR 701126CD-23146251725461871463486 18 41 51.6-23 50 006.23 Am
HR 7023BD-19 5134172816161754ID V3879 Sgr18 42 55.2-19 17 026.35 M4III 2.60.6D:Occultation double.,R:Occultation diam., two determinations, 0.0085" and 0.0101".,VAR:SRb 6.05 - 6.58p, about 50d.
HR 7026CD-3612946172875210507 18 44 07.7-36 43 076.32 K0III
HR 7029CD-35128761729102105093490W 18 44 19.4-35 38 314.87 B2.5V 7.89.4G:Sco-Cen assoc.; member of the Sco-Cen cluster; member of Pleiades group.
HR 7035CD-2513394173117187216D 18 44 49.6-25 00 405.83 B5:V 0.20.0D:Duplicity questionable.,G:Sco-Cen assoc.,SB:Suspected double, 6.4, 6.6v, sep. 0.04", probably SB.
HR 7038BD-21 5131173282187234 18 45 18.7-21 00 056.36 F5V
HR 7039φ27CD-27131701733001872391487D 18 45 39.4-26 59 273.17 B8III 0.00.1D:4.1, 4.1v, sep. 0.13", doubtful.
HR 7045BD-19 5154173425161803I 1130918 46 01.2-19 36 236.42 M4III R:Diam. 0.0039".,VAR:Amp. 0.15V.
HR 704628BD-22 4854173460187255I11652 18 46 20.6-22 23 325.37 K4III 7.713.7
HR 7070CD-3413128173902210600 18 49 17.2-34 44 556.62 K1IVCNIII
HR 7072BD-18 5079173928161848W 18 48 45.3-18 36 056.47 G5III:+A0V: 0.70.4
HR 7077BD-19 5182174115161871D Var?18 49 35.5-19 08 326.75 A1m 0.00.2D:Suspected occultation double.,VAR:6.69 - 6.82V.
HR 707829BD-20 5277174116187324I11713 1137218 49 40.1-20 19 295.24 K4III 8.616.6
HR 708830BD-22 4881174309187342149311731 18 50 50.5-22 09 446.61 A7III 6.821.1G:Hyades group.
HR 7103CD-2613562174630187388 18 52 28.5-26 39 016.29 G8/K0III
HR 7104CD-2915449174631187389 18 52 37.0-29 22 466.13 K1III
HR 7105CD-30163561746322106633502 18 52 41.7-30 44 036.63 B8V
HR 711433BD-21 5176174947187422I 18 54 00.1-21 21 355.69 K1Ib
HR 7116ν132BD-22 4907174974187426I11794 18 54 10.2-22 44 424.83 K2I+B9V: 5.82.5D:AB fixed, combined mag., colors. C, 11.21V, +1.25(B-V), +1.20(U-B), at 28".,N:Ain al Rami.
HR 7120ν235BD-22 4915175190187445I 18 55 07.1-22 40 174.99 K3II-IIIBa0.8CN2
HR 7121σ34CD-2613595175191187448706IW 18 55 15.9-26 17 482.02 B2.5V 7.4309.0C:Color excess E(B-V) = +0.02.,D:Interferometer measures indicate multiple star.,G:Sco-Cen assoc.,N:NUNKI; Sadira.,S:Lyman alpha and Lyman beta observed from COPERNICUS.
HR 7126BD-16 50781753171619841495 18 55 31.0-16 22 365.79 F4V
HR 7128CD-2314844175360187468 18 56 00.6-23 10 255.93 B8
HR 7145ξ136BD-20 5339175687187498 18 57 20.5-20 39 235.08 A0II
HR 7150ξ237BD-21 5201175775187504710I 18 57 43.8-21 06 243.51 K1III R:Occultation diam. = 0.0030 - 0.0042".
HR 7151CD-3116189175794210773 18 58 21.3-31 02 106.12 K3III
HR 7155CD-2513574175852187517D 18 58 20.5-24 52 366.62 A0 0.00.1D:Suspected occultation double, equal components.
HR 7159BD-22 4928175892187519 18 58 24.6-22 31 466.14 A2V
HR 7164BD-18 5155176123162050D 18 59 26.8-18 34 016.37 G3II D:Suspected occultation double.
HR 7166BD-13 5172176162162052W Var18 59 23.8-12 50 265.53 B5IV 0.50.4D:Binary. B1, B9.,VAR:Amp. 0.053B.
HR 7168CD-2513614176246187562 19 00 24.8-24 56 326.36 gK0
HR 7182BD-22 4946176537187584I 19 01 37.8-22 41 446.24 K5
HR 7186BD-15 5185176593162097 19 01 33.5-15 16 576.32 gG6
HR 7194ζ38CD-3016575176687187600I11950 19 02 36.7-29 52 492.60 A2III+A4IV 0.30.5D:AB 3.2 A2III, 3.4 A2V, 21.138y, a = 0.532".,DYN:0.040".,N:Ascella.
HR 7195CD-2513655176704187599D 19 02 27.7-24 50 495.65 K3III 0.00.1D:Suspected occultation double with equal components; combined mag., color.,G:Arcturus group.,R:Occultation diam. under 0.002".
HR 7203BD-19 527317688416213011972 19 03 03.8-19 14 436.05 G6III 3.57.4D:AB CPM. B, 9.17V, +0.47(B-V), +0.09(U-B).
HR 7205BD-19 5275176903162133D 19 03 07.0-19 06 126.37 F5IV-V 0.00.1D:Probable double, 7.1, 7.1v, sep. 0.05".
HR 7211CD-3116306177074210883 19 04 25.1-31 02 495.50 A0IV
HR 7217ο39BD-21 5237177241187643I11996 1170319 04 41.0-21 44 303.77 G9IIIb 9.935.7
HR 7230BD-15 52231775171621773522W Var?19 05 41.2-15 39 375.97 B9V 6.246.9S:Sp. shows Hg, Si.,VAR:Variable on short time scale with uncertain 0.33772d period. Manfroid and Mathys (1985, A&AS, 59, 429) also give,VAR:possible 0.48773d period. Magnetic field not detected (Borra and Landstreet 1980, ApJS, 42, 421).
HR 7234τ40CD-27135641777161876831496I 19 06 56.4-27 40 143.32 K1+IIIb G:Possibly Wolf 630 group.
HR 7239BD-16 515317781716220112039 19 06 52.3-16 13 446.03 B8IV 4.06.4D:Companion A0V.
HR 7240CD-2815403177846187701I 19 07 30.9-28 38 136.04 K3III
HR 7241BD-18 5206177863162204 1174319 07 08.5-18 44 166.29 B8III
HR 7246CD-2415041178075187718 19 08 14.6-24 39 256.30 B9III
HR 7249BD-19 5312178175162229 V4024 Sgr19 08 16.7-19 17 245.54 B2Ve vS:H alpha variable.,VAR:Amp. 0.2V.
HR 7256CD-36133551782992109963528 19 09 36.4-36 09 536.56 A0IV SB:Nearly equal components. Period probably long.
HR 7264π41BD-21 5275178524187756720IW 1176919 09 45.8-21 01 252.89 F2II 0.00.1D:AB, combined mag., colors, sep. 0.093". Third component 6.0v at 0.4".,G:Red star Pleiades group.,N:Albaldah; Al Baldah.
HR 7265BD-20 541517855516226012096 19 09 48.1-19 48 136.13 K1III 0.20.1D:7.0 K3III, 7.2 K2III. Unresolved by speckle interferometry. Probably not double.
HR 7270CD-2915804178840187786 19 11 18.9-29 30 086.30 B9
HR 7276BD-21 5292179201187816 19 12 28.0-21 39 296.41 gG8
HR 7277CD-26139361793231878353533I 19 13 13.7-25 54 245.80 K1I
HR 7282BD-12 53111794971623263534I 1181519 13 15.5-12 16 575.51 gK4
HR 7291CD-2415161179949187883 19 15 33.2-24 10 456.25 F9V
HR 7292ψ42CD-2513866179950187882I12214 19 15 32.4-25 15 244.85 G8:III+A8V 0.30.1C:Probably not IR source.,D:5.5 F8V, 5.7 F9V, 18.75y, a = 0.153". Component A is SB, 6.2, 6.2v, sep. 0.001".,DYN:0.010".,S:AB variously classified as F2:+F7III, F8V+F9V, F6V+F7V, A8V+G8:III.,SB:ADS 12214B, SB2O 10.7786d, K 72.5k/s, V0 -43.0k/s, asini 9.48. Masses 2.1 and 1.7 solar. ADS 12214AB, 7319.0d, K,SB:10.0k/s, V0 -26.8k/s, msin3i 3.78, asini 866. A, 2.7 solar mass.
HR 7296CD-3314076180093211117I RY Sgr19 16 32.8-33 31 186.25 G0Ipe(C1,0) C:Possible extinction by circumstellar dust.,M:Possibly high luminosity evolved helium star.,RV:38.6d.,S:Hydrogen deficient carbon star.,VAR:RCB 6.0 - >15.0v. Also pulsations 38.454d, changing amplitude. Observations 1984-86 indicate semiregular pulsations,VAR:of 33 to 40d, 6.13 - 6.78V, 0.38 - 0.76(B-V), -0.09 to +0.52(U-B).
HR 730443BD-19 5379180540162413722D 19 17 38.1-18 57 114.96 G8II-III D:Suspected occultation double.,R:Diam. 0.0018".
HR 7316CD-35133931808852111751501 19 19 40.0-35 25 175.59 B3V G:Sco-Cen assoc.; Sco-Cen cluster?
HR 7317BD-15 5310180928162462IW 19 19 00.1-15 32 116.06 K3III 5.548.6
HR 7323CD-3215071181109211191I 19 20 26.2-31 49 046.58 M0III
HR 7327BD-22 5063181240187992 19 20 38.1-22 24 095.58 F0III:
HR 7330CD-3513422181321211206 19 21 29.9-34 59 026.48 G5V VAR:Nearby star suspected of variability from photometric discordances by different observers.
HR 7334CD-4214133181401229643 19 22 09.6-42 00 586.34 K1III
HR 7337β1CD-44132771814542296461502W 19 22 38.3-44 27 324.01 B9V 3.328.3D:CPM. Companion A5V; vsini 129k/s, optical?,N:Arkab Prior; Arkab or Urkab with HR 7343.
HR 7339BD-19 5412181558162511W 19 21 37.1-19 14 036.26 B5V 3.690.8D:Component B, K2IV, RV -3; component C, G5:III, optical.
HR 7340ρ144BD-18 5322181577162512D Rho1 Sgr19 21 40.4-17 50 503.93 F0IV-V 2.50.0D:Sep. 0.036". Questionable occultation double.,G:Possible Eggen group with HR 63, q.v.,VAR:Delta Sct 3.90 - 3.93V, 0.050d.
HR 7342υ46BD-16 5283181615162518727ID Ups Sgr19 21 43.6-15 57 184.61 B2Vpe+A2IaShell v1.00.0C:Large IR excess.,S:Hydrogen deficient, strong carbon? Also classified B8+F2p, B8I, F0Ia, and Apep + O9V. H alpha variable.,SB:4.8, 5.8v, sep. 0.011", 137.9567d, K 49.1k/s, V0 +13.3k/s, asini 93.0. Analysis of IUE data by Dudley and,SB:Jeffery (1990, MNRAS, 247, 400) gives a K2 velocity of 29.7k/s and a mass ratio of 0.63+/-0.01, indicating that,SB:upsilon Sgr is a strong candidate as a progenitor of a type Ib supernova.,VAR:EB 4.34 - 4.44p, 137.939d. Irregularities in light variation. Variable polarization, probably due to circumstellar,VAR:dust.
HR 7343β2CD-4513171181623229654 19 23 13.2-44 47 594.29 F2III N:Arkab Posterior; Arkab or Urkab with HR 7337.
HR 7344ρ245BD-18 5325181645162521 19 21 50.9-18 18 305.87 gG9
HR 7348αCD-4013245181869229659728 19 23 53.2-40 36 583.97 B8V N:Rukbat; Rucba; Rukbat al Rami; Alrami.
HR 7350CD-4313352181925229660 19 24 21.4-43 43 236.17 M1-2III
HR 7355CD-2815767182180188079 19 24 30.1-27 51 566.04 B2Vn G:Sco-Cen assoc.
HR 7360CD-291610418228618809312400 19 25 04.1-29 18 335.93 K3III 4.412.1D:Optical.
HR 7362χ147CD-2415303182369188101W 19 25 16.5-24 30 315.03 Am 0.00.1D:5.8 A8, 5.8 A6-F0, 10.8y, a = 0.123". Probable occultation double. Speckle interferometry 1985.5 gives sep. 0.081".,N:Chi1 Fl 47, Chi2 Fl 48 and Chi3 Fl 49 Sgr are, respectively, HR 7362, HD 182391 (7.08v, B9) and HR 7363.,G:Hyades group.,S:K/H/met give A5/F0V/F0.
HR 7363χ349CD-2415307182416188105I 1199219 25 29.7-23 57 445.43 K4III
HR 7367BD-14 54281824771625953552I 19 25 21.6-13 53 495.69 K3III
HR 737550BD-22 51051826291881213553I 19 26 19.2-21 46 365.59 K3III
HR 7378BD-15 5348182645162609 19 26 11.1-15 03 115.72 B8Vn tVAR:H alpha emission variable.
HR 7379BD-14 5435182678162615 19 26 24.6-14 33 046.70 A1V
HR 7380CD-2916140182681188127731 19 26 56.5-29 44 365.67 B9V
HR 7392CD-4313395183007229712 19 29 23.9-43 26 455.71 Am S:Also classified A3p.,SB:164.64d, K 11.8k/s, V0 -30.9k/s, asini 26.5.
HR 7398CD-2714004183275188192I12506 19 29 52.2-26 59 085.52 K3III 3.57.6D:Binary. B, 8.69V, +0.86(B-V), +0.32(U-B), G1IV-V.,DYN:0.011".,G:Hyades group.,S:Also classified K2IIIab.
HR 7399CD-3215233183312211315 19 30 14.7-32 05 326.60 F3IV-V
HR 7410BD-21 5410183545188219 19 30 54.0-21 18 446.13 A2
HR 7422CD-40133561840352297463560 V4089 Sgr19 34 08.5-40 02 055.89 A3III SB:4.625d, K 72.5k/s, V0 +11.9k/s, asini 4.59. Masses 3 and 2 solar. Primary overluminous for its mass; secondary may,SB:be neutron star.,VAR:E, amp. 0.13V, 4.62988d.
HR 743151CD-2415442184552188326 1218319 36 01.7-24 43 095.65 A7m 2.00.0SB:5.9, 7.9v, sep. 0.0002", 8.1158d, K 20.9k/s, V0 -30.3k/s, asini 2.31.,VAR:Primary of SB Delta Sct? Amp. 0.015V in about 10d.
HR 7433BD-12 5461184574162797 19 35 33.6-12 15 106.27 K0
HR 7439BD-19 5521184705162809 19 36 26.1-18 51 106.11 F0III
HR 744052CD-251418418470718833773612654 1219119 36 42.4-24 53 014.60 B9 4.52.7D:CPM.,VAR:ADS 12654. Uncertain which component varies.
HR 7443BD-18 54321848351628163565 19 37 03.3-18 13 525.64 K3III
HR 7454BD-14 5479184985162827 19 37 34.4-14 18 065.47 F5V SB:Unresolved by speckle interferometry 1986.46.
HR 7464CD-3913371185257211451 V4090 Sgr19 39 55.7-39 26 006.61 A2m S:Also classified A7V.
HR 747053CD-231561818540418840712741 19 39 49.4-23 25 406.34 B9.5V+A3IV 0.20.2D:Sep. 0.200".
HR 7473CD-2315625185467188419 19 40 07.1-23 25 435.97 gK1
HR 747654BD-16 53991856441628831512I12767 A1227519 40 43.4-16 17 366.20 K2III+F8V 0.00.1D:Primary is close double, combined colors. Mag. for blend 5.30V. Component B, 12.6v at 38" optical. C, 8.9 F8V,D:at 46" physical.,VAR:Amp. 0.09V.
HR 748955BD-16 54131860051629151514W 19 42 31.1-16 07 265.06 F1III 0.00.2D:Suspected visual double, but may be single.
HR 7491CD-37133221860422115063576 19 43 37.6-37 32 206.16 B8
HR 7496BD-15 5444186185162931W 19 43 33.5-15 28 125.49 F5IV 6.270.4RV:Over 1500d.
HR 7507CD-32154431865002115411516 19 46 01.2-31 54 315.52 B8V
HR 751556BD-20 56981866481629641517I 19 46 21.7-19 45 404.86 K1III
HR 7532BD-14 5555186984162998 19 48 03.0-13 42 126.11 A6m
HR 7538CD-2916546187098188603358212956 19 49 11.6-28 47 206.05 F2V D:6.1, 11.9v sep. 2" in 1910, 1913, not seen as double in 1926, 1928, 1929. Probably single?
HR 7552CD-40135141874742299033583 V3961 Sgr19 51 50.6-39 52 285.33 A0pCrSr: vSB:690d.,VAR:5.28 - 5.33V, 2445.2d. Revised period 2300d. Variable magnetic field and spectrum.
HR 756157BD-19 5631187739163060 19 52 12.0-19 02 425.92 G5III
HR 7571BD-14 5578187949163080S V505 Sgr19 53 06.4-14 36 116.48 A0V+F8IV 0.3D:Speckle interferometry indicates companion at 0.291", probably not the same as the SB or occultation binary.,SB:6.6 - 8.6v, sep. 0.0002", 1.1829d, K 104k/s, V0 -2k/s, asini 1.69; vsini of secondary 50k/s.,VAR: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,VAR:both about 2.2.
HR 7578CD-241566818808818869213072 Var?19 54 17.7-23 56 286.18 K2V 4.031.5D:Optical.,SB:46.817d, e 0.692, K(A) 48.8 k/s, K(B) 48.7 k/s, V0 -5.1 k/s, m(A)sin3i = m(B)sin3i = 0.85,,SB:a(A)sini 22.7, a(B)sini 22.6.,VAR:BY Dra type predicted, but variability not yet detected.
HR 7581ιCD-42145491881142299271520 19 55 15.7-41 52 064.13 K0II-III
HR 7585CD-3314560188158211653 19 55 05.1-33 02 476.46 K2/3III
HR 7597ω58CD-2614637188376188722I 19 55 50.4-26 17 584.70 G5V N:Terebellum, name shared with HR 7604, 7618, 7650.
HR 760459CD-2714399188603188742I 19 56 56.8-27 10 124.52 K2.5IIb N:Terebellum, name shared with HR 7597, 7618, 7650.
HR 7605CD-3813776188642211686 19 57 41.3-38 03 306.55 F4V
HR 761461BD-15 55161888991631411522 19 57 57.0-15 29 295.02 A3IV
HR 7617CD-3017525188981211708 19 58 56.4-30 32 176.28 K1III
HR 761860CD-2614682189005188778I 19 58 57.2-26 11 444.83 G6IIIBa0.2 N:See HR 7597.
HR 7623θ1CD-3513831189103211716751 19 59 44.2-35 16 354.37 B3IV G:Member of the local association (Pleiades group).,SB:2.1051d, K 15.9k/s, V0 +0.9k/s, asini 0.460.
HR 7624θ2CD-3513832189118211717W 19 59 51.3-34 41 525.30 A4/5IV 5.530.
HR 7627CD-4313735189140229977 20 00 26.5-43 02 366.14 M0II-III
HR 7629CD-3813802189195211719W 20 00 15.9-37 42 085.95 G8III 7.623.0
HR 7630CD-45135491891982299813597 20 00 48.3-45 06 475.81 A8III S:Also classified F0/2IV.
HR 7631CD-3414082189245211724 1265520 00 20.3-33 42 145.66 F7V SB:Unresolved by speckle interferometry 1986.46.,VAR:Amp. 0.07V.
HR 7639CD-4113807189388229993 20 01 26.4-40 48 516.29 A2-3V
HR 7643CD-23159351895611888293600 20 01 23.9-22 44 146.01 G7V
HR 764963BD-14 5618189741163195 20 01 58.6-13 38 135.71 A3V
HR 765062CD-2816355189763188844753I V3872 Sgr20 02 39.5-27 42 354.58 M4III C:May not be the IR source.,N:See HR 7597.,VAR:L? 4.45 - 4.61V.
HR 7652CD-38138281898312117673602 20 03 33.5-37 56 274.77 K5III G:Hyades group; Zeta Her group.
HR 7658BD-22 5318190009188863D 20 03 44.3-22 35 446.45 F6V D:Suspected occultation double.
HR 7659CD-32156821900562117823606IW 1274620 04 19.6-32 03 234.99 K1III 7.651.3
HR 7668CD-3314700190306211798W 20 05 32.1-33 00 006.53 B8 1.00.4
HR 767565BD-13 5569190454163253 20 05 26.4-12 39 556.55 A1Vn
HR 7703CD-3613940191408211885W 20 11 11.9-36 06 045.32 K3V 4.0D:AB CPM. B, 11v dM5, sep. 6.6". Wroclaw contr. no. 16 gives mag. differences but no sep. for four components: AB 5.4v,,D:AC 5.15, and AD 4.0. Possible misidentification? Discovered by John Herschel as simply double. Components C and D,D:apparently first listed by van Albada at Lembang in 1958; only magnitudes and no separations were indicated.
HR 7706CD-4313855191584230100 20 12 23.9-42 46 506.22 K1III
HR 7725CD-30177731924332119403621 20 15 50.6-30 00 196.30 K4III
HR 7728CD-3614011192472211948W 1294920 16 23.7-36 27 166.39 M4III 5.138.0
HR 7729CD-3514020192486211950 20 16 26.5-35 11 526.53 F2V
HR 7764CD-291698119328118916413702 20 20 28.1-29 11 506.30 A4/7V 1.127.2C:Combined mag. and color of AB and C.,D:Component C, photometric spectral class A2IV, vsini 53k/s. Component B, 10.1V at 4.1". For component AB, Rakos and,D:Mermilliod give 6.93V, +0.28(B-V), +0.24(U-B). However, other sources give the following V magnitudes:,D:Comp. 1976 1978 1980 Preferred,D:Gronbech and Oblak Ruffener,D:Olsen,D:AB 6.635 6.610 6.608 6.61,D:C 7.724 7.706 7.72,D: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).,S:Photometric spectral class A2III.
HR 7765CD-36140571933022120251530 20 20 51.9-35 40 256.46 K3-4III
HR 7779κ1CD-4214836193571230177763W 20 22 27.5-42 02 595.59 A0V 6.052.0
HR 7787κ2CD-4214847193807230184W 20 23 53.2-42 25 225.64 A5V 0.90.6D:AB binary. Combined mag., colors.,DYN:0.011".
HR 7799CD-4114024194184230197 20 25 47.9-40 47 476.09 K3III SB:117.776d, K 22.6k/s, V0 +42.1k/s, asini 35.5.
HR 7801CD-29170491942151892641532D 20 25 26.8-28 39 485.85 G8II/III SB:377.60d, K 11.2k/s, V0 -7.3k/s, asini 58.0.
HR 7808CD-3713741194433212126W 20 26 53.0-37 24 116.25 K2IV-V 1.41.1D:6.6 K2IV-V, 7.8 K1V, 232.76y, a = 1.225".,DYN:0.024".

Legende

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)

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