Catalogues

Cancer / Yale Bright Star Catalog (HR)

«Yale Bright Star Catalogue, 5th Revised Ed.» Hoffleit D., Warren Jr W.H., 1991 [154]
HRBFDMHDSAOFK5IRM*ADSVarIDRADecvMagspTypedMagSepRemarks
HR 30951BD+16 159064960973991208I 07 56 59.4+15 47 255.78 K3+III
HR 3104BD+16 15986525797429ID 07 58 31.5+16 31 075.99 K0 0.00.2D:Occultation double.
HR 3115BD+13 18116552297445I 07 59 35.1+13 14 326.02 K2
HR 3124ω12BD+25 181265714798611211 08 00 55.9+25 23 345.83 gG8
HR 3125BD+20 19766573597471 08 00 48.0+19 48 586.25 K1III
HR 3127BD+23 186665757798646513 08 01 00.7+23 34 596.34 R K1III-IV 4.52.3
HR 31283BD+17 173165759974722618I 08 00 47.3+17 18 315.55 gK3 R:Occultation diameter = 0.0040".
HR 3132ω24BD+25 18166585679869W 08 01 43.8+25 05 236.31 A1V 3.8109.3
HR 31345BD+16 16126587397485 08 01 30.3+16 27 195.99 B9.5Vn
HR 3158BD+19 19116655297537 08 04 45.2+18 50 326.15 R B9V
HR 31638BD+13 183166664975422625 08 05 04.5+13 07 055.12 A1V
HR 3164BD+27 153666684799286569 3892 08 05 37.0+27 31 476.21 A0V 0.73.7D:Binary. Combined light and colors.,RV:ADS 6569B, -15k/s.
HR 3169μ19BD+23 18876687579940I BL Cnc08 06 18.4+22 38 085.99 M3III VAR:Lb 5.97 - 6.04V.
HR 3176μ210BD+22 186267228799592630I 08 07 45.8+21 34 545.30 G1IVb
HR 318412BD+14 18316748397594 08 08 42.4+13 38 276.27 F3V
HR 3191ψ14BD+25 186567767799952633W 08 10 27.2+25 30 265.73 G7V 4.9112.1G:Wolf 630 group.,N:Psi2 Fl 14 Cnc. Psi1 Fl 13 is HD 67690 (6.7v, K0). HR 3191 also called simply Psi Cnc.
HR 3198BD+15 17756795997628 08 10 58.8+14 37 466.23 A1V
HR 3201BD+10 174668099116444 08 11 16.6+09 49 166.07 B6III M:Old disk population runaway star.
HR 3208ζ116BD+18 186768257976456650 A08 12 12.7+17 38 525.63 F8V 0.40.9D:Combined mag. and color for 3208-9-10, 4.67V, +0.53(B-V). AB 5.63 F7V, 6.02 F9V combined colors (AB), 59.7y,,D:a = 0.884". Component C = HR 3210.,DYN:0.039".,N:Tegmen; Tegmine.
HR 3209ζ116BD+18 186768256976456650 B08 12 12.7+17 38 526.02 F9V 0.40.9D:See HR 3208. ABxC, 1150y, a = 7.96".
HR 3210ζ216BD+18 186768255976466650 C08 12 13.3+17 38 526.20 G5V 1.25.9D:See HR 3208. C* 6.20 G5V, 17.5y, a = 0.191". Astrometric companion also found by occultation, 9.0v. Cc resolved by,D:speckle interferometry.,DYN:0.031".
HR 3214BD+14 18506833297647 08 12 22.1+14 00 146.54 A7III
HR 321515BD+30 166468351800162641 BM Cnc08 13 08.9+29 39 245.64 B9pSiCr N:15 Cnc is also Psi Gem, in Cancer.,SB:585.4154d, K 12.1k/s, V0 +17.8k/s, asini 94.6.,VAR:Alpha CV 5.53 - 5.65V, 4.116d.
HR 3222BD+16 16626846197653D 08 12 59.8+16 30 516.01 G8III D:Suspected occultation double.
HR 3224BD+23 19136854380024 08 13 41.7+23 08 166.56 A4IVn
HR 3228BD+18 188268703976696673 08 14 11.1+17 40 336.47 A0VnDel Del 3.063.0
HR 3231BD+13 18686877697671W 08 14 21.0+13 02 546.38 G8III 5.622.8
HR 3248BD+12 18036924397694I R Cnc08 16 33.9+11 43 357.13 M7IIIe P:Polarization possibly due to circumstellar dust scattering.,S:SiO maser.,VAR:M 6.2 - 11.8v, 361.43d.
HR 3249β17BD+09 191769267116569312I6704 3973 08 16 30.9+09 11 083.52 K4IIIBa0.5 9.429.2D:CPM.,N:Altarf; Al Tarf.
HR 3252BD+09 192169478116585 08 17 31.7+08 51 586.29 G8III
HR 3262χ18BD+27 158969897801041217 08 20 03.9+27 13 045.14 F6V
HR 3264BD+21 181769994801122646 08 20 21.0+20 44 525.83 K1III
HR 3268λ19BD+24 19097001180113 08 20 32.1+24 01 205.98 R B9.5V
HR 328420BD+18 193070569977811220 08 23 21.8+18 19 565.95 A9V
HR 329021BD+11 18307073497788I6787 08 23 55.2+10 37 556.08 M2III 3.31.0
HR 329925BD+17 18427103097806 08 25 49.9+17 02 466.14 F6V
HR 3304φ122BD+28 160271093801812656IW 08 26 27.7+27 53 375.57 K5III 4.3130.6
HR 3306BD+08 20537111511675226556805 08 25 54.8+07 33 525.13 G7II-IIIFe-1 5.230.4
HR 3310φ223BD+27 161271150801876815 B4078 08 26 46.8+26 56 046.32 H A6V 0.15.2D:Binary with HR 3311. Colors for combined light.
HR 3311φ223BD+27 161271151801886815 A4078 08 26 47.0+26 56 076.30 H A3V 0.15.2D:See HR 3310.
HR 331224BD+25 192071152801846811 A4076 08 26 39.8+24 32 037.02 F0III 0.65.7D:Binary with HR 3313.,N:BAC and some old catalogues call 24 CNC = Upsilon1; HR 3329 = 28 = Upsilon2; HR 3355 = 30 = Upsilon3.,N:Most modern catalogues follow Heis identifications: HR 3355 = 30 = Upsilon1; HR 3369 = 32 = Upsilon2.
HR 331324BD+25 192071153801856811 B4076 08 26 40.1+24 32 077.81 F7V 0.65.7D:BC 8.6 dF6, 8.6, 21.82y, a = 0.19". Also binary with A, HR 3312.
HR 331927BD+13 191271250978192658I BP Cnc08 26 43.9+12 39 165.50 M3III G:Arcturus group.,VAR:SRb 5.41 - 5.75V, about 40d.
HR 332928BD+24 19317149680204 CX Cnc08 28 36.8+24 08 416.10 F0Vn VAR:Delta Sct, amp. 0.025V, 2.3 hours.
HR 333329BD+14 189971555978431222D 08 28 37.3+14 12 395.95 A5V 0.50.2D:Uncertain if double or triple; 6.4, 6.9, sep. 0.25", other possible component 7.0v at 3". Occultation obs. uncertain.
HR 3355υ130BD+24 194072041802292666 08 31 30.5+24 04 525.75 F0IIIn
HR 3357θ31BD+18 196372094978812667IW 4117 08 31 35.7+18 05 405.35 K5III 0.00.3D:Occultation pair 6.4, 6.4v, blended mag. and colors. Visual component 10v at 63". Suspected as double by Innes from,D:observation of occultation of April 28, 1898 (references: Astron. Nachr. 150, 423, 1899; MNRAS, 61, 416, 1901;,D:Cape Ann. 2, part 6, 1907).,VAR:Theta Cnc B is NSV 4117, 11.5v at 58", 59d.
HR 3361BD+10 181672208116863 08 31 54.6+09 48 526.83 B9p:Hg:
HR 3366η33BD+20 21097229280243321I 08 32 42.5+20 26 285.33 K3III
HR 3369υ232BD+24 19467232480245 08 33 00.1+24 05 056.36 G9III G:61 Cyg group.
HR 337234BD+10 18187235997902 08 32 39.9+10 03 586.46 A1V
HR 3376BD+13 19407250597913D 08 33 45.1+13 15 266.28 K0III 0.00.1
HR 3380BD+08 207772617116894W 08 34 13.3+08 27 076.03 F3IV 7.631.2
HR 338735BD+20 21187277997928 08 35 19.4+19 35 246.58 G0III G:NGC 2632 #1133; Praesepe.
HR 3394BD+15 18517294397950 08 36 07.7+15 18 496.32 F0IV
HR 3395BD+07 1997729451169296886 A08 35 51.0+06 37 125.99 F8V 1.210.3D:CPM with HR 3396.,DYN:0.008".,SB:ADS 6886A, 14.296d, K 22.7k/s, V0 +24.2k/s, asini 4.28.
HR 3396BD+07 1997729461169316886 B08 35 51.3+06 37 217.25 G5V 1.210.3D:See HR 3395.,DYN:0.008".
HR 340636BD+10 1837731431169532675 08 37 05.8+09 39 205.88 A3V
HR 3409BD+33 17287319260939 08 38 19.0+32 48 075.94 gK2
HR 341237BD+10 184073316116975 08 38 05.2+09 34 296.53 A1V
HR 3423BD+32 17767359660970 08 40 18.3+31 56 316.10 R F5III
HR 3424BD+08 209973599116997 08 39 24.6+08 01 026.45 K1III
HR 342739BD+20 21587366580333W 4179 08 40 06.4+20 00 286.39 G8III 0.0149.8D:Components B, 6.60V, +0.01(B-V), +0.03(U-B), A0III at 150", vsini =<40k/s; P, 9.22V, +0.39(B-V), +0.01(U-B) at 134"; and,D:Q, 8.81V, +0.32(B-V), +0.09(U-B), F2V, at 135", vsini 86k/s, form a physical system with A. B is 40 Cnc; Q is +20d2161.,G:In Praesepe; NGC 2632 #253.,S:Also classified K0III.
HR 3428BD+20 216673710980216921 08 40 22.1+19 40 126.44 G9III 1.363.2D:ACD a physical group: C, 7.70V, +0.20(B-V), +0.16(U-B), Am, vsini <45k/s. D, 9.39V, +0.41(B-V), +0.03(U-B), F5V at,D:83". B, 10.37V, +0.59(B-V), +0.11(U-B), G0IV-V at 21", CPM.,G:NGC 2632 #283.,S:Also classified K0III.
HR 3429ε41BD+20 21717373198024W 08 40 27.0+19 32 426.30 A8Vn 1.1134.9G:In Praesepe; NGC 2632 #300.,S:Also classified A5m, Am (K/H/M) = A7/A8/F0, and Am (A5/F0/F1).
HR 3449γ43BD+21 189574198803781228W 08 43 17.1+21 28 074.66 A1IV 4.0106.3D:Component A suspected occultation double. Three visual companions.,G:Hyades group.,N:Asellus Borealis.
HR 345045BD+13 197274228980692686 08 43 12.3+12 40 515.64 A3V+G0III 0.00.1SB:72.99d, K1 24.4k/s, K2 41.0k/s, V0 -0.9k/s, asini 24.0; unresolved by speckle interferometry. vsini of,SB:secondary 70k/s.
HR 3461δ47BD+18 20277444298087326I6967 08 44 41.1+18 09 153.94 K0III-IIIb 7.538.4D:AP, suspected double, unresolved by speckle interferometry. Visual companion 12.2v at 38" optical.,N:Asellus Australis.
HR 346446BD+31 187674485610292690 08 45 21.4+30 41 526.13 G5III G:UMa stream.,N:BAC and Heis (Argelander) differ on the correspondence between Flamsteed numbers and Bayer letters. The Heis convention,N:is adopted here. The corresponding interpretations are as follows: HR, FL, Heis, BAC; 3464, 46, -, Sigma1;,N:3519, 51, Sigma1, -; 3532, 57, -, Sigma2; 3555, 59, Sigma2, -; 3563, 61, -, Sigma3;,N:3575, 64, Sigma3, -. In the Bayer atlas (1603) the letter Sigma is in a position between these two groups,N:(BAC being south of Heis configurations) and could apply just as well to either. Most older catalogues give the BAC,N:convention.
HR 346549BD+10 186474521980892688 BI Cnc08 44 45.0+10 04 545.66 A1pEuCr G:Pleiades group.,S:Magnetic star.,VAR:Alpha CV 5.58 - 5.71V, 4.2359d.
HR 3474ι48BD+29 18237473880415I6988 B4238 08 46 40.0+28 45 556.57 A3V 2.530.4D:Binary with HR 3475.,DYN:0.023".,VAR:The magnitude difference between HR 3474 and 3475 appears to vary.
HR 3475ι48BD+29 18247473980416328I6988 A4238 08 46 41.8+28 45 364.02 G7.5IIIaBa0.1 2.530.4D:Binary with HR 3474.,DYN:0.023".,S:Also classified G8II.,VAR:Probably NSV 4238.
HR 348150BD+12 19047487398117 08 46 56.0+12 06 365.87 A1V
HR 3504BD+19 21107546998162 08 50 45.1+18 49 566.16 R A2V s
HR 351054BD+15 191775528981682699D 08 51 01.5+15 21 026.38 G1V 1.40.1D:Sep. 0.05", but duplicity doubtful.
HR 3519σ151BD+33 177075698611027057 08 52 34.6+32 28 275.66 A8Vma s 4.479.0N:See HR 3464.
HR 352153BD+28 16597571680476IW BO Cnc08 52 28.6+28 15 336.23 M3III 3.543.1N:BAC and others call this Rho1, HR 3522 Rho2, and HR 3540 Rho3.,RV:Lines of higher excitation potential show higher RV.,S:Magnetic star.,VAR:Lb? 6.23 - 6.37V.
HR 3522ρ155BD+28 16607573280478 08 52 35.8+28 19 515.95 G8V 7.085.0D:CPM.,G:Hyades group.,N:See HR 3521.,S:Enhanced CN and C2 and perhaps CH.
HR 353257BD+31 19077595961125I7071 08 54 14.7+30 34 465.39 G7III 0.21.5D:AB binary. B is K0.,N:See HR 3464.
HR 3540ρ258BD+28 166676219805112705I 08 55 39.7+27 55 395.22 G8II-III N:See HR 3521.
HR 3541BD+17 19737622198230I X Cnc08 55 22.9+17 13 536.64 C6II R:Occultation diam. = 0.0079".,VAR:SRb 5.6 - 7.5v, 9.3 - 10.9p, 195:d.
HR 355060BD+12 19417635198235ID 4308 08 55 55.6+11 37 345.41 gK5 D:Suspected occultation double.,R:Occultation diam. = 0.0033".
HR 3555σ259BD+33 17857639861146 08 56 56.6+32 54 375.45 A7IV N:See HR 3464.
HR 3558BD+17 19797650898245 08 57 08.2+17 08 386.17 K1III
HR 3561ο162BD+15 19457654398247 08 57 14.9+15 19 225.20 A5III
HR 356361BD+30 179576572611577107 08 57 58.7+30 14 016.29 F6V 0.00.1D:7.0, 7.0v; combined mag., colors. Unresolved by speckle interferometry.,N:See HR 3464.
HR 3565ο263BD+16 18647658298250 08 57 35.2+15 34 535.67 F0IV
HR 3567BD+09 2093766291173012710 08 57 42.0+09 23 166.19 G8III
HR 3572α65BD+12 194876756982673377115 4327 08 58 29.2+11 51 284.25 A5m 0.00.1D:ADS 7115A is questioned close double. Combined mag., colors, 5.0, 5.0v, sep. 0.1". B is 10.8v at 11", binary.,DYN:0.029".,G:Sirius group?,N:Acubens; Sertan; Sartan.,S:Spectrum shows phosphorus.
HR 3575σ364BD+32 182176813611771232IW 08 59 32.6+32 25 075.20 G8III 3.889.3N:See HR 3464.
HR 3577BD+18 20937683098276I 4332 08 59 10.8+18 08 056.38 M4III v
HR 358766BD+32 182977104612027137 09 01 24.1+32 15 095.82 R A2V 2.34.6D:AB fixed.
HR 358967BD+28 16747719080585W 09 01 48.9+27 54 106.07 A8Vn 2.8103.5S:Shell star. Possible weak emission on violet wing of H alpha. Shell spectrum not always present.
HR 3595ν69BD+25 202977350805952714 4356 09 02 44.3+24 27 105.45 A0pSi vG:Sirius group? UMa stream.,S:HgMn star. Also classified A0pSrCr.,SB:1401.4d, K 7.7k/s, V0 -14.3k/s, asini 139.,VAR:Alpha CV 5.33 - 5.49V. Spectral-line intensities vary with period 4.191d.
HR 3599BD+07 206677445117369 09 02 44.8+07 17 535.85 gK3
HR 360170BD+28 16837755780609 09 04 09.9+27 53 546.38 R A1V
HR 3606BD+32 18377766061242 09 04 55.2+32 22 376.46 A8V
HR 3617BD+23 204878175806437187 A09 07 26.9+22 58 526.40 F4V 0.47.6D:AB binary. B is F5V. C, optical.,DYN:0.015".
HR 3620BD+33 18107823461276 09 08 04.1+32 32 266.50 F2V
HR 3621τ72BD+30 181778235806502719 09 08 00.1+29 39 155.43 G8III
HR 3623κ76BD+11 198478316983781238D Kap Cnc09 07 44.8+10 40 055.24 B8IIIpMn 0.20.3D:Triple SB system. Combined mag., colors.,S:Spectrum shows phosphorus. Magnesium deficient relative to oxygen. Gallium II lines strong. Normal SiII, weak MgII.,S:Lambda Boo type. HgMn star. It has been suggested that a nearby supernova explosion could have produced reactions,S:to account for abundance anomalies.,SB:6.3933d, K 67.4k/s, V0 +24.5k/s, asini 5.88. 5.8 - 7.8v, sep. 0.0003" and 6.0, sep. 0.3".,VAR:Alpha CV 5.22 - 5.27V, 5.0035d.
HR 362675BD+27 171578418806592724W 09 08 47.3+26 37 455.98 G5IV-V 3.1112.0SB:19.4589d, K 20.2k/s, V0 +12.3k/s, asini 5.28; 19.412d, K1 26.6k/s, K2 33.6k/s, V0 10.4k/s,,SB:a1sini 6.95, a2sini 8.73.
HR 3627ξ77BD+22 206178515806661239W 09 09 21.5+22 02 445.14 G9IIIFe-1CH-0.5 0.50.1D:Unresolved by speckle interferometry.,S:Also classified K0III.,SB:1700.76d, K 4.4k/s, V0 -7.7k/s, asini 103.
HR 3635BD+12 19797866198400 09 09 46.4+11 33 526.48 F2Vp
HR 3639BD+31 19467871261306I RS Cnc09 10 38.7+30 57 475.95 M6IIIase S:Technetium star. CO emission. OH radio emission.,VAR:SRc? 6.2 - 7.7p, 120d. Mean mag. varies in period 1700d.
HR 364079BD+22 20637871580674W 09 10 20.9+21 59 476.01 G5III 0.00.1D:Unresolved by speckle interferometry.
HR 3650π181BD+15 20037909698427W 09 12 17.6+14 59 466.51 G9V 0.00.1D:AP 7.2 G9V, 7.2 G9V, 2.65y, a = 0.126". Resolved by speckle interferometry 1983.94, sep. 0.17". Combined mag.,,D:colors.
HR 3657BD+21 19917924880702 09 13 37.3+21 17 006.48 A2V
HR 3669π282BD+15 200979554984562733I 09 15 13.8+14 56 295.34 K1III N:Usually called Pi Cnc.
HR 3689BD+12 200980064984767285 09 17 51.4+11 30 046.41 A2IV 5.921.8D:Optical.
HR 3707BD+33 18488054661424 09 21 27.2+32 54 076.16 K3III
HR 3711BD+15 20278061398517 09 21 15.4+15 22 166.53 A1V

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