Catalogues

Aries / 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 522 4 BD+16 203 10982 92637 1050 01 48 10.9 +16 57 20 5.84 B9.5V
HR 530 1 BD+21 243 11154 74966 1457 01 50 08.5 +22 16 31 5.86 K1III+A6V 1.1 2.8 D:Binary. Component B 7.3v A6V, P.A. 166d; RV, 1.8k/s, variable. Confusion in literature as to which component is HD,D:11154, which 11155. Probably combined mag. and color.,DYN:0.006".,G:UMa stream.
HR 534 BD+10 252 11257 92659 D 635 01 50 52.0 +11 02 36 5.94 F2V w 0.0 0.1 G:UMa stream.,N:54 Cet in Aries.
HR 545 γ1 5 BD+18 243 11503 92680 1507 B Var? 01 53 31.8 +19 17 45 4.83 H B9V v 0.1 7.8 D:Binary with HR 546, q.v. Combined mag. HR 545/6, 3.88V; colors also combined.,DYN:0.019".,N:The HD numbers and other data, especially spectral classes, for HR 545-6 have frequently been interchanged. HD 11502 is,N:the brighter = HR 546, while HD 11503 = HR 545 is the slightly fainter N. prec. component B of ADS 1507.,VAR:Sp. var. 38 min.
HR 546 γ2 5 BD+18 243 11502 92681 1507 A Gam Ari 01 53 31.8 +19 17 37 4.75 H A1pSi 0.1 7.8 D:Binary with HR 545, orbital period 5000 - 10000y? Component C, 9.6v at 221". Combined colors for HR 545-6; combined,D:mag. 3.88V.,DYN:0.019".,G:Pleiades group.,N:Mesarthim; Mesartim; "First Star in Aries".,S:Also classified A0pCr, A1pCrSiSr.,VAR:Alpha CV 3.88 - 3.90V, 2.6095 or 1.7982d; also possibly 2.5 hrs., amp. 0.02, unconfirmed. Southern component of,VAR:ADS 1507. Magnetic var.
HR 553 β 6 BD+20 306 11636 75012 66 I 658 01 54 38.4 +20 48 29 2.64 A5V N:Sharatan; Sheratan; Al Sharatain.,SB:106.9973d, K 37.1k/s, V0 -4.0k/s, asini 23.8. One of the most eccentric orbits known: e 0.892. Binary unresolved by,SB:speckle interferometry 1981.69. SB2 in infrared: near-IR reticon spectra at 8800 Ang show double lines and indicate,SB:that the secondary is late F- or G-type main-sequence star.,VAR:Delta Sct?
HR 559 7 BD+22 284 11763 75030 2130 I RR Ari 01 55 51.0 +23 34 38 5.74 K1III VAR:EA? 6.42 - 6.84p, 47.9?d.
HR 563 ι 8 BD+17 289 11909 92721 2132 I 01 57 21.1 +17 49 03 5.10 K1p 1.0 0.0 S:Also classified G2Ib-II.,SB:1567.66d, K 10.8k/s, V0 -4.9k/s, asini 217, 5.4, 6.4v, sep. 0.01", unresolved by speckle interferometry.
HR 569 λ 9 BD+22 288 11973 75051 1563 A 680 01 57 55.7 +23 35 46 4.79 F0V 2.5 37.4 D:ADS 1563B, 7.40V, +0.58(B-V), +0.07(U-B), dG1, CPM; vsini =<25k/s.,VAR:ADS 1563B; Cst? 7.30 - 740V.
HR 577 BD+20 322 12139 75077 1582 D 01 59 35.7 +21 03 30 5.87 K0III-IV 3.3 188.1 D:ADS 1582AB, 8.5, 11.0v, sep. 2.3" at 188" from the bright component D. C, 9.2v at 31" from A.
HR 578 BD+11 261 12140 92739 2136 01 59 25.9 +12 17 41 6.09 A6V
HR 601 BD+12 271 12479 92763 I 02 02 35.2 +13 28 36 5.94 M2III R:Occultation diam., two determinations, 0.0026" and 0.0036".
HR 605 10 BD+25 341 12558 75114 1631 02 03 39.3 +25 56 08 5.63 F8IV 1.5 0.8 D:AB 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,D:925y. Combined mag., colors.,DYN:0.016".
HR 609 BD+17 307 12594 92774 I D 02 03 42.6 +18 15 12 6.21 gK4 D:Suspected occultation double.
HR 613 κ 12 BD+21 279 12869 75146 02 06 33.9 +22 38 54 5.03 A2m SB:15.2938d, K 34.4k/s, V0 +11.5k/s, msin3i 0.137, asini 5.75.
HR 615 11 BD+25 349 12885 75149 1658 02 06 49.2 +25 42 17 6.15 B9IV-Vn 5.5 1.6
HR 617 α 13 BD+22 306 12929 75151 74 I 725 02 07 10.4 +23 27 45 2.00 K2-IIICa-1 N:HAMAL; Hemal; Hamul; Ras Hammel; El Nath (obsolete). The name Arietis also used both for the star and the constellation.,S:Also classified K2IIIab Ca-1.
HR 623 14 BD+25 355 13174 75171 W 02 09 25.3 +25 56 23 4.98 F2III 2.5 105.9
HR 624 BD+16 247 13201 92810 02 09 23.1 +17 13 28 6.43 F5V
HR 631 15 BD+18 277 13325 92822 1056 I 738 02 10 37.6 +19 30 01 5.70 M3IIIab
HR 633 16 BD+25 362 13363 75188 I 02 11 12.0 +25 56 13 6.02 gK4
HR 644 BD+23 297 13522 75203 I 02 12 37.5 +24 10 04 5.96 K0
HR 646 η 17 BD+20 348 13555 75204 02 12 48.1 +21 12 39 5.27 F5V M:Possible nearby star on basis of spectroscopic parallax.
HR 648 19 BD+14 357 13596 92841 1057 I 748 02 13 03.3 +15 16 47 5.71 M0III G:Zeta Her group.
HR 656 20 BD+25 373 13871 75239 02 15 46.0 +25 46 59 5.79 F6IV-V G:Hyades group; Mel 25 #157.
HR 657 21 BD+24 329 13872 75238 1059 W 02 15 42.8 +25 02 35 5.58 F6V 0.3 0.2 D: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,D:interferometric sep. 0.17", 1983.93.,M:Possible nearby star on basis of spectroscopic parallax.
HR 665 BD+23 307 14067 75262 2156 02 17 10.4 +23 46 04 6.55 G9III
HR 669 θ 22 BD+19 340 14191 92877 81 02 18 07.5 +19 54 04 5.62 A1Vn
HR 676 BD+22 329 14262 75277 02 18 58.0 +23 10 04 6.46 A1V+F3III SB:363.51d, K 19.4k/s, V0 -24.64k/s, asini 91.5; vsini of secondary 110k/s.
HR 702 ξ 24 BD+09 316 14951 92932 2164 02 24 49.0 +10 36 38 5.47 B7IV
HR 711 BD+26 409 15152 75370 I 02 27 07.0 +27 00 48 6.18 K5III
HR 723 BD+22 354 15385 75398 02 29 13.6 +23 28 08 6.19 A5m
HR 728 BD+24 358 15524 75407 2171 1904 02 30 32.4 +25 14 06 5.92 F6IV 4.5 113.1 D:ADS 1904AB binary; B, 11v.
HR 729 26 BD+19 365 15550 92979 2172 D UU Ari 02 30 38.4 +19 51 19 6.15 A9V D:Suspected occultation double.,S:Also classified A9III.,VAR:Delta Sct 6.11 - 6.15V, 0.080d.
HR 731 27 BD+17 380 15596 92983 1069 02 30 54.4 +17 42 14 6.23 G5III-IV
HR 741 29 BD+14 419 15814 92998 2176 02 32 54.1 +15 02 05 6.04 F8V
HR 763 31 BD+11 360 16234 93022 2179 D 02 36 37.9 +12 26 51 5.68 F7V 0.1 0.0 D:Sep. 0.021".
HR 764 30 BD+24 375 16232 75470 1982 B 02 36 57.7 +24 38 54 7.09 F4V 0.6 38.3 D:CPM with HR 765. HR 764 formerly misidentified as the SB = HR 765. Data for HR 764 and 765 have frequently been,D:interchanged.
HR 765 30 BD+24 376 16246 75471 1982 A 02 37 00.5 +24 38 51 6.50 F6III 0.6 38.3 D:CPM with HR 764.,G:Hyades group.,SB:ADS 1982A, 1.1095d, K 22.4k/s, V0 +14.4k/s, asini 0.341.
HR 773 ν 32 BD+21 362 16432 75495 89 02 38 49.0 +21 57 41 5.43 A7V
HR 782 33 BD+26 443 16628 75510 2033 02 40 41.1 +27 03 39 5.30 A3V 4.2 28.6 D:CPM.
HR 793 μ 34 BD+19 403 16811 93062 2062 02 42 22.0 +20 00 42 5.69 R A0Vnp: 0.8 0.1 D: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,D:resolved by speckle interferometry, sep. 0.045" 1981.68, 0.040" 1981.69.,S:Lambda Boo star, Mg 4481 wk:
HR 797 BD+10 360 16861 93067 899 02 42 28.9 +10 44 30 6.30 A2V G:UMa stream.,VAR:Delta Sct?
HR 801 35 BD+27 424 16908 75532 94 02 43 27.1 +27 42 26 4.66 B3V G:Cas-Tau OB1.,SB:490d. Short period 2.6d not confirmed. K 8.8, V0 +13.0, asini 58.7.
HR 803 BD+25 441 16955 75539 2082 02 43 51.2 +25 38 17 6.35 A2Vp: 4.1 2.9 D:AB CPM.,S:Lambda Boo star, Mg 4481 wk:
HR 808 36 BD+17 426 17017 93081 2190 02 44 19.1 +17 45 50 6.46 K2III G:Wolf 630 group.
HR 809 ο 37 BD+14 457 17036 93082 02 44 32.9 +15 18 42 5.77 B9Vn
HR 812 38 BD+11 377 17093 93083 UV Ari 02 44 57.6 +12 26 45 5.18 A7III-IV VAR:Delta Sct 5.18 - 5.22V, 0.0355d with overtones of 0.046 and 0.061d.
HR 824 39 BD+28 462 17361 75578 I 02 47 54.5 +29 14 50 4.51 K1.5III
HR 828 40 BD+17 442 17459 93118 I D 937 02 48 32.1 +18 17 01 5.82 K1III 0.0 0.2 D:Suspected occultation double, 6.8, 6.8v, sep. 0.2".,G:Probable Hyades group.
HR 830 BD+24 396 17471 75588 VZ Ari 02 48 45.9 +25 11 17 5.86 R A0V S:Also classified ApSi.,VAR:Alpha CV, 5.82 - 5.89V.
HR 836 π 42 BD+16 355 17543 93127 2151 944 02 49 17.5 +17 27 51 5.22 B6V 3.0 0.0 D:AB 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,D:pair with computed sep. 0.00004".,SB:ADS 2151A, 3.854d, K 24.8k/s, V0 +7.8k/s, asini 1.31.
HR 838 41 BD+26 471 17573 75596 100 2159 951 02 49 59.0 +27 15 38 3.63 B8Vn 4.8 124.9 D:Optical system.,G:Pleiades group.
HR 847 σ 43 BD+14 480 17769 93144 1079 02 51 29.6 +15 04 55 5.49 B7V
HR 856 BD+15 400 17918 93164 02 53 11.7 +16 29 00 6.31 F5III
HR 867 ρ2 45 BD+17 457 18191 93189 RZ Ari 02 55 48.5 +18 19 54 5.91 M6-III: N:Rho1 Fl 44, Rho2 Fl 45, Rho3 Fl 46 Ari are, respectively, HD 18091 (6.93v, A3), HR 867 and 869. HR 869 is,N:also called simply Rho Ari.,R:Occultation diam. = 0.0095 - 0.012".,VAR:SRb 5.62 - 6.01V, 30d.
HR 869 ρ3 46 BD+17 458 18256 93195 2204 02 56 26.1 +18 01 23 5.63 F6V SB:3507d, K 6.7k/s, V0 +12.1k/s, asini 308. Orbit questioned by Morbey and Griffin (1987, ApJ, 317, 343).,SB:Unresolved by speckle interferometry 1978.96.
HR 878 47 BD+20 480 18404 75662 1081 02 58 05.2 +20 40 07 5.80 F5IV G:Hyades group.
HR 887 ε 48 BD+20 484 18519 75673 2257 B 1001 02 59 12.7 +21 20 25 4.63 A2V s 0.3 1.5 D:Binary with HR 888. Mag. and colors for combined light.,DYN:0.012".,VAR:Uncertain if HR 887 or 888 is the variable suspect.
HR 888 ε 48 BD+20 484 18520 75673 2257 A 1001 02 59 12.7 +21 20 25 4.63 A2V s 0.3 1.5 D:A, 5.25H; B = HR 887, 5.55H; C, 12.7v at 146".,DYN:0.012".
HR 902 BD+10 401 18700 93232 2213 I 03 00 44.1 +10 52 13 5.95 K6
HR 905 49 BD+25 477 18769 75693 2214 1021 03 01 54.1 +26 27 44 5.90 A3m
HR 916 BD+27 468 18928 75709 03 03 30.3 +28 16 11 6.36 F0V
HR 924 BD+15 430 19080 93260 03 04 40.7 +15 51 22 6.49 R K3III
HR 927 52 BD+24 431 19134 75723 2336 A 03 05 26.7 +25 15 19 6.80 B7V 0.0 0.2 D:Binary with HR 928. Colors for combined light. AB, 227y, a = 0.470". Triple system with C, 10.8v at 5".,RV:Probably blended with HR 928.
HR 928 52 BD+24 431 19135 75723 2336 B 03 05 26.7 +25 15 19 7.00 B7V 0.0 0.2 D:See HR 927.,RV:Probably blended with HR 927.
HR 931 BD+12 436 19270 93276 2220 03 06 23.7 +13 11 14 5.62 K3III
HR 938 53 BD+17 493 19374 93284 D UW Ari 03 07 25.7 +17 52 48 6.11 B1.5V 0.0 0.0 D:Sep. 0.03".,M:Runaway star from Ori OB1 association at 59k/s. Presumably originated in Ori 1 assoc. Its space vel. is twice that of,M:HR 1712 = AE Aur and opposite that of HR 2688. These three stars and HR 1996 (Mu Col) appear to be receding from an,M:HII shell of about 110000 solar masses expanding at 10k/s.,SB:0.15275d. Amp. and V0 variable.,VAR:Beta C 6.10 - 6.23V, 0.15275d. Possibly a SN 4.9 million yrs. ago.
HR 940 54 BD+18 414 19460 93293 I 03 08 21.2 +18 47 42 6.27 M0III R:Diam. 0.0021".
HR 944 55 BD+28 499 19548 75757 1088 03 09 36.7 +29 04 37 5.72 B8III G:Member of the local association (Pleiades group).
HR 945 BD+27 480 19600 75762 03 10 08.8 +27 49 12 6.42 A0V v VAR:Constant light but large H-line variation.
HR 946 BD+26 516 19637 75771 03 10 27.0 +26 53 47 6.02 K3III
HR 948 BD+11 445 19698 93320 D 03 10 38.9 +11 52 21 5.98 B8V D:Suspected occultation double.
HR 951 δ 57 BD+19 477 19787 93328 114 I 1066 03 11 37.8 +19 43 36 4.35 K2III v G:Hyades group.,N:Botein.
HR 952 BD+12 452 19789 93327 D 03 11 21.9 +13 02 52 6.12 K0IIIp D:Suspected occultation double.
HR 954 56 BD+26 523 19832 75788 SX Ari 03 12 14.2 +27 15 25 5.79 B9pSi v RV:Period 0.728d probably rotation period. Earlier determination vsini 94k/s.,VAR:SX Ari 5.67 - 5.81V, 0.7278925d. Spectral variations (SiII, HeI, same period). Possible 30 min Sp. var.,VAR:suggesting star spots related to magnetic field. Silicon abundance varies 10 to 100 times solar, and magnesium 0.03 to,VAR:10 times solar.
HR 971 BD+30 512 20149 56285 03 15 20.5 +30 33 24 5.52 R A1V s
HR 972 ζ 58 BD+20 527 20150 75810 1089 03 14 54.1 +21 02 40 4.89 A1V
HR 995 59 BD+26 540 20618 75863 03 19 55.8 +27 04 16 5.90 G6IV
HR 999 BD+28 516 20644 75871 2234 I 03 20 20.4 +29 02 54 4.47 K2II-III
HR 1000 60 BD+25 536 20663 75875 03 20 25.6 +25 39 46 6.12 gK3
HR 1005 τ1 61 BD+20 543 20756 75886 1094 W 03 21 13.6 +21 08 49 5.28 B5IV 2.5 0.2 D:Suspected of being double or triple by Tebbutt in 1893. Components 5.4, 7.9v, sep. 0.15", and 8.4v at 0.67".,G:Cas-Tau OB1.
HR 1012 62 BD+27 500 20825 75892 03 22 11.9 +27 36 27 5.52 G5III
HR 1015 τ2 63 BD+20 551 20893 75899 I 03 22 45.2 +20 44 31 5.09 K3III
HR 1022 64 BD+24 481 21017 75912 2240 I 03 24 18.5 +24 43 27 5.50 gK4
HR 1027 65 BD+20 556 21050 75915 03 24 26.1 +20 48 13 6.08 A1V
HR 1048 66 BD+22 495 21467 75945 2552 03 28 26.6 +22 48 15 6.03 K0IV 1.4 0.0 D:ADS 2552A is close binary, 6.3, 7.7v, sep. 0.010". AB binary; C, 13v at 148".

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