Catalogues

Capricornus / Yale Bright Star Catalog (HR)

«Yale Bright Star Catalogue, 5th Revised Ed.» Hoffleit D., Warren Jr W.H., 1991 [154]
HR B F DM HD SAO FK5 IR M* ADS VarID RA Dec vMag spType dMag Sep Remarks
HR 7694 BD-10 5285 191110 163290 20 08 31.3 -10 03 46 6.18 B9.5III S:Peculiar star of Hg type.,SB:9.3464d, K 51.5k/s, V0 -8.4k/s, msin3i 0.654, asini 6.62.
HR 7709 BD-09 5382 191639 144144 3618 Var 20 11 10.1 -08 50 32 6.49 B1V VAR:Amp. 0.3V, 0.09U, 16.82d. Magnetic var.
HR 7712 ξ1 1 BD-12 5664 191753 163328 20 11 57.9 -12 23 33 6.34 K0III
HR 7715 ξ2 2 BD-13 5608 191862 163337 W 20 12 25.9 -12 37 03 5.85 F7V 6.2 71.6
HR 7722 CD-2714659 192310 189065 12933 20 15 17.4 -27 01 58 5.73 K0V v
HR 7738 3 BD-12 5680 192666 163402 13600 20 16 22.8 -12 20 13 6.32 B9pHg 7.3 26.9
HR 7747 α1 5 BD-12 5683 192876 163422 1527 I 13632 20 17 38.9 -12 30 30 4.24 G3Ib 0.4 377.7 D: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.,N:Prima Giedi; Algiedi Prima; Algedi with HR 7754.
HR 7748 4 BD-22 5384 192879 189114 1529 20 18 01.4 -21 48 36 5.87 K0III
HR 7754 α2 6 BD-12 5685 192947 163427 761 I 13645 20 18 03.3 -12 32 41 3.57 G8IIIb 0.4 377.7 D:IDS notes Alpha1 Cap = HR 7747 (ADS 13632, four components) as one of five components of Alpha2 Cap = HR,D:7754 = ADS 13645. Hence, we have recorded n = 9 for both. ADS 13645AB optical; BC 11.2, 11.5v, sep. 1.2" binary.,N:Secunda Giedi; Algiedi Secunda; Gredi; Algedi, with HR 7747.
HR 7761 σ 7 BD-19 5776 193150 163445 3625 I 13675 20 19 23.6 -19 07 07 5.28 K3II 3.5 56.5
HR 7773 ν 8 BD-13 5642 193432 163468 13714 20 20 39.8 -12 45 33 4.76 B9.5V 7.0 54.1 D:CPM.,N:Alshat.,R:Occultation diam. = 0.0028 - 0.0036".
HR 7775 BD-15 5626 193452 163471 13717 20 20 46.6 -14 47 06 6.10 A0III 0.3 0.0 D: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,,D:sep. 0.05". Component B, 10.2v, A1, binary with A at 0.9". A is astrometric binary. The close occultation pair is,D:questioned; it has not been confirmed by speckle interferometry.,SB:ADS 13717A = component B of multiple star of which HR 7776 is component A. 8.6780d, K 37.9k/s, asini 4.22. These are,SB:components BC of triple spectroscopic system with HR 7776. BC sep. 0.0225", mag. diff 1.1. BC could be eclipsing.,SB:Component C of the spectroscopic triple system is not the same as any of the visual components of ADS 13717 listed by,SB:Worley; nor is it component C of the components Worley lists for HR 7776 = STF 52.
HR 7776 β 9 BD-15 5629 193495 163481 762 I W 20 21 00.7 -14 46 53 3.08 F8V+A0 0.3 0.0 D:Complex system with HR 7775, q.v. Component B, vsini 97k/s. Occultations indicate component A is multiple system: 4.0,,D: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,D:two faint 13v components at 112" discovered by John Herschel.,N:Dabih. Beta1 = Dabih Major; Beta2 = Dabih Minor.,R:Occultation diam. = 0.00305 - 0.00317". Diam. primary 0.0033".,S:Also classified G0III + B8V, K0II-IIIp + A0, B8V + K0II-III, or G8II + A0V:.,SB:HR 7776-7775 = AxBC. 1374.126d, K 21.9k/s, V0 -18.9k/s, msin3i 3.75, asini 376. Alternate orbit 1374.23d,,SB:K 22.44k/s, V0 -18.95k/s, msin3i 3.63, asini 382.5. Might be eclipsing. vsini of sceondary 115k/s?
HR 7788 BD-10 5369 193896 144361 3632 20 23 00.8 -09 39 17 6.30 G5IIIa
HR 7814 π 10 BD-18 5685 194636 163592 13860 20 27 19.2 -18 12 42 5.25 B8II-III 3.4 3.3 D:AB CPM.
HR 7819 BD-16 5609 194918 163612 20 28 43.6 -15 44 30 6.41 K0III
HR 7822 ρ 11 BD-18 5689 194943 163614 13887 20 28 51.6 -17 48 49 4.78 F2IV 1.7 249.5 D:AB binary. B, 8.0v at 0.8".,DYN:0.017".,G:Sirius group.
HR 7825 BD-22 5442 195006 189345 3639 I 20 29 31.3 -22 23 30 6.16 M1III
HR 7829 ο 12 BD-19 5830 195093 163625 13902 B 20 29 52.5 -18 35 12 6.74 A7V 0.8 21.9 D:CPM with HR 7830.
HR 7830 ο 12 BD-19 5831 195094 163626 13902 A 20 29 53.9 -18 35 00 5.94 A3Vn 0.8 21.9 D:CPM with HR 7829.
HR 7837 BD-15 5696 195330 163645 W 20 31 04.3 -15 03 23 6.12 gG5+F 0.0 0.1 D:Also observed as occultation double, 6.6, 7.4v, sep. 0.1".
HR 7842 CD-2514854 195549 189416 20 32 52.4 -24 56 38 6.36 A0
HR 7845 BD-10 5423 195564 163665 1536 13960 20 32 23.7 -09 51 12 5.65 G2.5IV 4.2 103.2 D:AB, CPM. B, 11.3v at 3".
HR 7855 BD-14 5781 195838 163686 3645 20 34 11.7 -13 43 16 6.13 F6V
HR 7865 BD-17 6027 196078 163712 20 35 32.2 -16 31 33 6.19 A7V
HR 7877 CD-2514920 196385 189503 20 37 52.1 -25 06 32 6.36 F0III
HR 7889 τ 14 BD-15 5743 196662 163771 14099 20 39 16.4 -14 57 17 5.22 B6III 0.6 0.3 D:AB 5.8 B6III, 6.3 B6IV, 200y, a = 0.31". Visual third component 13v at 159". Occultation fourth companion, 9.3V, sep.,D:0.052".,N:Tau1 Fl 13 and Tau2 Fl 14 Cap are, respectively, HD 196348 (6.76V, K3III) and HR 7889, the former being,N:in the BS Supplement. HR 7889 is usually called simply Tau Cap.
HR 7898 CD-2416193 196761 189549 20 40 11.7 -23 46 26 6.37 G8V
HR 7900 υ 15 BD-18 5738 196777 163779 773 I 20 40 03.0 -18 08 19 5.10 M2III R:Occultation diam. = 0.0041 - 0.0086".
HR 7902 CD-2714959 196815 189559 20 40 36.0 -26 38 42 6.51 F7V
HR 7905 BD-16 5663 196857 163783 20 40 32.5 -16 07 27 5.80 gG7
HR 7910 CD-2615192 196947 189575 20 41 24.1 -26 00 00 6.28 K2III
HR 7931 CD-2715014 197540 189641 20 45 13.2 -27 14 50 6.50 G8III
HR 7936 ψ 16 CD-2515018 197692 189664 779 20 46 05.7 -25 16 15 4.14 F4V
HR 7937 17 BD-22 5523 197725 189667 3659 20 46 10.0 -21 30 51 5.93 A0
HR 7961 CD-2615282 198174 189733 20 49 17.6 -25 46 53 5.86 B7IIIp
HR 7964 BD-18 5783 198208 163910 3663 I W 20 49 20.5 -18 02 09 6.21 K3III 6.5 31.6
HR 7980 ω 18 CD-2715082 198542 189781 1546 I 13351 20 51 49.3 -26 55 09 4.11 M0-III-IIIbBa0.2 G:UMa stream.,S:Also classified M0-III-IIIbBa0.2.
HR 7989 CD-2416328 198732 189801 14380 20 53 01.2 -23 46 59 6.33 K0III 2.1 1.8 D:CPM. G8III-IV + G2.5IV.
HR 8000 19 BD-18 5805 199012 163975 I 20 54 47.9 -17 55 23 5.78 K0III
HR 8013 CD-2615344 199260 189856 13412 20 56 47.3 -26 17 47 5.70 F7V
HR 8018 BD-16 5741 199443 164013 1548 20 57 40.6 -16 01 54 5.87 A2m S:Also classified A7IV/V.
HR 8033 20 BD-19 5982 199728 164043 AO Cap 20 59 36.1 -19 02 07 6.25 B9pSi VAR:Alpha CV, amp. 0.050V, 2.25d.
HR 8045 CD-2715197 200052 189942 21 01 45.3 -26 52 52 6.05 A7V:m: S:K line slightly weak? Also classified A3V.
HR 8060 η 22 BD-20 6115 200499 189986 W 21 04 24.3 -19 51 18 4.84 A5V 1.3 0.3
HR 8075 θ 23 BD-17 6174 200761 164132 1552 21 05 56.8 -17 13 58 4.07 A1V SB:840.6d, asini 160.
HR 8080 24 CD-2515235 200914 190025 791 I 14632 21 07 07.7 -25 00 21 4.50 M0.5III 7.1 26.2
HR 8083 BD-18 5862 201057 164156 13549 21 07 44.6 -17 27 19 6.17 A0V
HR 8087 χ 25 BD-21 5933 201184 190050 3690 W 21 08 33.6 -21 11 37 5.30 A0V 5.7 67.0
HR 8091 27 BD-21 5940 201352 190069 13566 21 09 33.0 -20 33 23 6.25 F1IV
HR 8122 BD-17 6216 202261 164249 21 15 06.6 -17 20 42 6.04 G5
HR 8127 φ 28 BD-21 5974 202320 190173 I 21 15 37.9 -20 39 06 5.24 gG9
HR 8128 29 BD-15 5935 202369 164263 I 13620 21 15 44.9 -15 10 17 5.28 M3III G:Hyades group.
HR 8137 30 BD-18 5903 202671 164286 D 21 17 57.3 -17 59 07 5.43 B8III 0.0 0.1 S:Sp. shows Mn. Helium-weak star.,SB:Suspected SB, 6.1, 6.1v, sep. 0.1".
HR 8139 31 BD-18 5904 202723 164289 21 18 15.7 -17 27 44 7.05 F2V
HR 8148 CD-2615541 202940 190236 14847 21 19 45.8 -26 21 11 6.56 G5V 3.0 2.5 D:AB binary. B is K4. Components D and E, 12v at 247" and 149" probably optical.,DYN:0.049".,SB:ADS 14847A, 21.3462d, K 24.0k/s, V0 -17.2k/s, asini 6.82.
HR 8167 ι 32 BD-17 6245 203387 164346 1561 I 21 22 14.8 -16 50 04 4.28 G7IIIFe-1.5
HR 8172 CD-2316877 203475 190285 I 21 23 00.5 -22 40 08 5.60 M1III
HR 8183 33 BD-21 6007 203638 190295 3707 I 13683 21 24 09.6 -20 51 07 5.41 K0III G:Wolf 630 group.
HR 8184 CD-2316889 203639 190293 21 24 07.9 -22 44 49 6.38 gK0
HR 8204 ζ 34 BD-2215388 204075 190341 806 I 14971 21 26 40.0 -22 24 41 3.74 G4Ib 8.6 21.3 N:DM is CoD (star moved from -23d zone to -22d zone between 1855 and 1875). In Southern Durchmusterung extension,N:(Schoenfeld 1886), SD-23d442.,S:BaII star. Overabundance of praseodymium. White dwarf companion.
HR 8207 35 BD-21 6020 204139 190349 I 21 27 14.8 -21 11 46 5.78 K5III G:UMa stream.
HR 8212 BD-12 6005 204363 164415 21 28 13.9 -11 34 06 6.61 F3V
HR 8213 36 BD-22 5692 204381 190374 I 21 28 43.4 -21 48 26 4.51 G5III N:DM is CoD.,S:Also classified G7IIIbCN-0.5Fe-1.
HR 8222 BD-19 6107 204577 164433 21 29 59.6 -19 08 52 6.57 F0V
HR 8235 CD-2515479 204943 190423 3720 21 32 33.3 -24 35 26 6.43 A7V
HR 8245 37 BD-20 6237 205289 190461 21 34 51.0 -20 05 04 5.69 F1V
HR 8247 CD-2416729 205342 190469 21 35 15.9 -23 27 15 6.40 gG7
HR 8260 ε 39 BD-20 6251 205637 164520 3724 W Eps Cap 21 37 04.8 -19 27 58 4.68 B2.5Vpe v 1.3 0.0 D:Component A is SB, 5.0, 6.3v, 0.0047"; component B, 9.5v K1III-IV: at 68", physical, vsini =<54k/s.,S:Shell star. Shell spectrum resembles supergiant A-type with vsini 50k/s. Also classified B3IIIe.,VAR:Gamma Cas 4.44 - 4.72V. Polarization variable. Slight variation in H alpha line width.
HR 8273 BD-11 5640 206005 164555 3728 21 39 28.1 -10 34 37 6.08 K0
HR 8278 γ 40 BD-17 6340 206088 164560 812 I 21 40 05.5 -16 39 44 3.68 F0p G:Hyades group.,N:Nashira.,S:Violet part of spectrum indicates luminosity III; G-band region, V; SrII4077 very strong, indicating luminosity II.,S:Also classified Am.
HR 8283 42 BD-14 6102 206301 164580 I 21 41 32.9 -14 02 51 5.18 G1V+G0V 2.0 0.0 G:Wolf 630 group.,SB:5.5, 7.5v, sep. 0.0008", 13.17399d, K 23.2k/s, V0 -1.3k/s, asini 4.1314. RV also varies in a longer period.,SB:Unresolved by speckle interferometry.
HR 8285 41 CD-2317057 206356 190559 I 15223 21 42 00.8 -23 15 46 5.24 G9III 6.2 5.1 D:CPM.
HR 8288 κ 43 BD-19 6152 206453 164593 I 21 42 39.5 -18 51 59 4.73 G8III
HR 8293 BD-20 6270 206546 164601 21 43 13.5 -19 37 15 6.22 A3m 0.1 0.0 G:Hyades group.,S:Violet region of spectrum indicates luminosity III; G-band region, V.,SB:6.9, 7.0v, sep. 0.001", 6.3702d, K 82.1k/s, V0 -25.5k/s, msin3i 1.62, asini 7.19.
HR 8295 44 BD-15 6046 206561 164600 D 21 43 04.4 -14 23 59 5.88 F0IV D:Suspected occultation double.
HR 8302 45 BD-15 6052 206677 164612 21 44 01.0 -14 44 58 5.99 F0V
HR 8311 46 BD-09 5829 206834 145637 I 21 45 00.3 -09 04 57 5.09 G8II-III
HR 8318 47 BD-09 5833 207005 145648 I AG Cap 21 46 16.3 -09 16 33 6.00 M3III R:Occultation diam. = 0.0028".,VAR:SRb 5.90 - 6.14V, about 25d.
HR 8319 λ 48 BD-12 6087 207052 164639 818 21 46 32.1 -11 21 57 5.58 A1V
HR 8322 δ 49 BD-16 5943 207098 164644 819 I 15314 Del Cap 21 47 02.4 -16 07 38 2.87 Am v 2.0 0.0 D:ADS 15314A. Component A is SB, 3.2, 5.2v, 0.0018"; B, 15.8v, 69"; C 12.7v, 120".,N:Deneb Algedi; Deneb Algiedi; Scheddi; Sheddi.,S:Delta Sct spectrum. Also classified Delta Del, A7mIII.,SB:1.0228d, K 70.8k/s, V0 -0.2k/s, asini 0.996.,VAR:EA (possibly RS CVn type) 2.83 - 3.05V, 1.0227789d. Form of light curve varies.
HR 8337 BD-13 6027 207503 164679 21 49 41.1 -12 43 23 6.31 A3m SB:vsini both components 20k/s.
HR 8340 BD-17 6389 207552 164686 21 50 13.1 -16 50 41 6.38 K0
HR 8346 BD-19 6176 207760 164697 21 51 41.8 -18 37 23 6.16 F0III
HR 8351 μ 51 BD-14 6149 207958 164713 1577 21 53 17.8 -13 33 06 5.08 F1III S:Also classified F0-2V.
HR 8355 BD-10 5785 208008 164717 W 21 53 36.0 -10 18 42 6.59 B9V 0.5 0.1 D:Occultation third component 8.8v at 0.02"; AB, sep. 0.114" by Finsen, 0.090-0.093" by speckle interferometry.
HR 8378 BD-21 6131 208735 190786 3757 I 21 58 43.8 -21 10 58 6.12 M4III

Legend

Key to columns [154]
HR Harvard Revised Number = Bright Star Number
B Bayer designation (greek letter)
F Flamsteed number
DM Durchmusterung Identification (BD = Bonn; CD = Cordoba; CP = Cape Photographic)
HD Henry Draper Catalog Number
SAO SAO Catalog Number
FK5 FK5 star Number
IR I 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;)
ADS Aitken's Double Star Catalog (ADS) designation
VarID Variable star identification
RA Right Ascension (J2000.0)
Dec Declination (J2000.0)
vMag Visual magnitude
spType Spectral type
dMag Magnitude difference of double, or brightest multiple
Sep Separation of components in Dmag if occultation binary (arcsec)
Remarks Note 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