Kataloge

Pisces / Yale Bright Star Catalog (HR)

«Yale Bright Star Catalogue, 5th Revised Ed.» Hoffleit D., Warren Jr W.H., 1991 [154]
HRBFDMHDSAOFK5IRM*ADSVarIDRADecvMagspTypedMagSepRemarks
HR 2BD-01 45256128569 00 05 03.8-00 30 116.29 gG9
HR 333BD-06 6357281285721002I Var?00 05 20.1-05 42 274.61 K0IIIbCN-0.5 2.50.0SB:72.93d, K 16.4k/s, V0 -6.6k/s, asini 15.8. Spectroscopic triple 5.0, 7.5v, 0.00003", third component 7.5v,SB:at 0.002".,VAR:Amp. 0.05V.
HR 11BD-03 2315128595 Var?00 07 44.1-02 32 566.43 B8IIIpSi N:4 Cet in Psc.
HR 14BD-03 33521286022006I AP Psc00 08 12.1-02 26 526.07 K2III+F 2.00.0D:SB1. Blue companion?,N:5 Cet in Psc.,SB:6.5 K2III, 8.5v F:, sep. 0.002", 96.41d, K 23.8k/s, V0 +1.1k/s, asini 31.3.,VAR:Giant eclipsing binary. Amp. =>0.2V. Period close to SB. Also classified as ellipsoidal var.
HR 2634BD+10 856091750122 00 10 02.3+11 08 445.51 B9Vn e4.47.7D:Companion 9.44V, +0.34(B-V), -0.14(U-B), G5Ve.,S:H and K lines in emission, lithium strong.
HR 29BD-06 11587128621D 00 10 18.8-05 14 555.84 K1III D:Suspected occultation double.
HR 5035BD+08 191061109087191 UU Psc00 14 58.8+08 49 155.79 F0IV 0.00.0D:Component A is SB. ADS 191B, 7.3v dA7 at 12". Period apsidal motion, 3y. Possible radio binary.,SB:ADS 191A, 0.8417d, K 89.9k/s, V0 +2.6k/s, msin3i 0.295, asini 1.04, equal masses. 6.6, 6.6v, sep. 0.0003".,VAR:Ell 6.0 - 6.03V, 0.841678d.
HR 5936BD+07 2712271091002015 00 16 34.1+08 14 246.11 G8II-III
HR 67BD+00 2813671091192017 00 17 47.7+01 41 206.17 K0II
HR 69BD+10 25141991832 00 18 17.2+11 12 216.05 K0III
HR 8041BD+07 3616351091521008I 132 00 20 35.9+08 11 255.37 gK3
HR 81BD+10 32166391858287 00 20 54.5+10 58 376.56 A0V 0.20.6D:B9.5, A2.
HR 8642BD+12 251796918662020303 00 22 25.5+13 28 576.23 K3III 4.628.9D:Optical.
HR 94BD-03 4920231287432021 00 24 29.7-02 13 096.07 K1III
HR 9744BD+01 5721141091921010W 00 25 24.2+01 56 235.77 G5III D:Suspected double probably single.,G:Sirius group?
HR 10347BD+17 55241191910I TV Psc00 28 02.9+17 53 355.06 M3III vG:Zeta Her group; Hyades group.,VAR:SR 4.65 - 5.42V, 49d, replaced by cycles 70 - 85d.
HR 10648BD+15 632436919121012I 00 28 12.7+16 26 426.06 K5III
HR 107BD+09 4724541092242028 00 28 20.1+10 11 236.04 F6Va vw G:Wolf 630 group.
HR 13152BD+19 792910740842033452 00 32 35.5+20 17 405.38 K0III 6.849.6
HR 13251BD+06 6429131092622032449 Var?00 32 23.8+06 57 205.67 B9.5V 0.70.0D:ADS 449A is triple occultation system, 6.2, 6.9v, sep. 0.031"; third component 8.8v at 0.196". ADS 449B, 9.7v at 27.5".,D:AB are CPM.,RV:Early determination of vsini 260k/s.,VAR:Suspect eclipsing because invisible at time of occultation.
HR 141BD+12 57316691980 00 34 55.3+13 22 166.40 K0
HR 145BD+12 59326891990 00 35 54.7+13 12 246.41 F7V
HR 15553BD+14 763379919952039 AG Psc00 36 47.3+15 13 545.89 B2.5IV vVAR:Beta CMa, amp. 0.035V, 0.096d. Different cycles show different amplitudes, from 0.002 to 0.036V. Doubt has been,VAR:expressed that this is due to interference between different periods. RV also shows amplitude changing from a few to,VAR:25k/s. Line profiles also vary.
HR 161BD+02 8034571093152040 00 37 30.5+03 08 076.39 K4III G:Sigma Pup group.
HR 16654BD+20 85365174175W 245 00 39 21.8+21 15 025.87 K0+V 4.9122.0VAR:5.83 - 5.89V.
HR 16755BD+20 87369074182I558 00 39 55.6+21 26 185.36 K0III+F3V 3.26.6D:Binary.,DYN:0.007".
HR 21157BD+14 111440892072I 293 00 46 33.0+15 28 325.38 M4IIIa VAR:Lb?, 5.32 - 5.45V.
HR 21358BD+11 964482920802050 00 47 01.5+11 58 265.50 G8II
HR 21459BD+18 1014490920822051 XX Psc00 47 13.6+19 34 446.13 F0Vn G:Hyades group.,VAR:Delta Sct? 5.99 - 6.03V, 0.1040d.
HR 21660BD+05 1044526109461 00 47 23.6+06 44 275.99 G8III
HR 21761BD+20 105456874280 00 47 54.8+20 55 316.54 F8V G:Hyades group.
HR 22162BD+06 1054627109470 00 48 17.4+07 18 005.93 G8III
HR 222BD+04 12346281094711019W 00 48 23.0+05 16 505.75 K2V 4.6181.2
HR 224δ63BD+06 107465610947428IW 00 48 41.0+07 35 064.43 K4IIIb 8.6113.3R:Occultation diam. = 0.0042".
HR 22564BD+16 764676920991020W 00 48 58.7+16 56 265.07 F8V 7.476.7D:The two companions probably optical.,SB:13.824581d, K 57.53k/s, V0 +4.06k/s, msin3i 1.041, asini 10.9; vsini both components <17k/s.
HR 23065BD+26 131475774295683 B00 49 52.8+27 42 397.00 F4III 0.04.5C:Colors for blend with HR 231. Mag. for blend, 5.56V.,D:CPM with HR 231.,DYN:0.004".,G:Hyades group.
HR 23165BD+26 131475874296683 A00 49 53.2+27 42 377.10 F5III 0.04.5D:CPM with HR 230.,DYN:0.004".,G:Hyades group.
HR 243BD+02 1184928109507 00 51 18.3+03 23 066.37 K0III G:Wolf 630 group.
HR 25466BD+18 122526792145746 00 54 35.2+19 11 185.74 R A1VN 0.80.5D:AB 6.23 A1V, 6.89 A4V, 360.4y, a = 0.700". Combined mag., colors.,DYN:0.011".
HR 259BD+23 126531674365I 346 00 55 14.7+24 33 256.20 M4IIIab
HR 26267BD+26 1515382743732059 00 55 58.5+27 12 346.09 A5IV
HR 27468BD+28 1575575743951023I 00 57 50.2+28 59 325.42 gG6
HR 276BD+12 119561292183 00 57 54.5+13 41 456.32 G8III G:UMa stream.
HR 277BD+20 131564174402805 00 58 18.9+21 24 166.37 R A2V 1.40.4D:ADS 805, 790y.
HR 284BD+05 1315820109581IW WW Psc00 59 49.7+06 28 596.11 M2III 7.131.0VAR:Lb 5.95 - 6.12V.
HR 291σ69BD+31 168611854374 01 02 49.1+31 48 165.50 B9.5V SB:81.12d, K 54.3k/s, V0 +10.4k/s, msin3i 0.547, asini 26.4.
HR 294ε71BD+07 153618610962736ID 01 02 56.6+07 53 244.28 K0III 0.00.2D:Suspected occultation double, 5.2, 5.2v, sep. 0.25".
HR 303BD+28 174630174471 01 04 27.6+29 39 316.19 F7IV-V
HR 30773BD+04 1726386109656I 01 04 52.6+05 39 236.00 gK5
HR 30872BD+14 1636397922301028889 01 05 05.4+14 56 465.68 F4II-III 7.455.2D:Visual pair optical.,S:Luminosity variously classified as II, III, V.,SB:ADS 889A.
HR 310ψ174BD+20 156645674482899 A397 01 05 40.9+21 28 245.34 A1Vn 0.329.9D:CPM with HR 311. Third component optical.
HR 311ψ174BD+20 157645774483899 B01 05 41.7+21 27 555.56 A0Vn 0.329.9D:CPM with HR 310.
HR 31377BD+04 1756479109666903 A01 05 49.2+04 54 306.35 F3V 1.033.0D:CPM with HR 314. Faint companions probably optical.,G:Wolf 630 group.
HR 31477BD+04 1766480109667903 B01 05 51.4+04 54 347.25 F6V 1.033.0D:CPM with HR 313.,G:Wolf 630 group.
HR 31975BD+12 1356557922502068 01 06 33.6+12 57 226.12 G8III
HR 32778BD+31 1856680544452072 01 08 01.3+32 00 446.25 F5IV G:Hyades moving group.
HR 328ψ279BD+19 185669574506 01 07 57.2+20 44 215.55 A3V
HR 33080BD+04 19067631096972073W 410 01 08 22.2+05 38 595.52 F0III-IV 3.8159.3D:Companions probably optical.,G:UMa stream.,VAR:Delta Sct?
HR 339ψ381BD+18 153690392283 Var?01 09 49.2+19 39 315.55 G0III
HR 341BD+24 186695374530I 01 10 19.4+25 27 285.80 K7III
HR 344BD+14 175696692288I 01 10 11.5+15 40 276.06 M0III
HR 34982BD+30 181703454493 01 11 06.8+31 25 295.16 F0V
HR 351χ84BD+20 1727087745441032I 01 11 27.2+21 02 054.66 G8.5III-IIIa
HR 352τ83BD+29 19071067454643I 01 11 39.6+30 05 234.51 K0.5IIIb
HR 356BD+29 195722974561990 01 12 59.5+30 03 516.19 G9III+G1V 4.110.8D:AB CPM. Component B, 10.25V, +0.79(B-V), +0.29(U-B), G1V.
HR 360φ85BD+23 1587318745712082I995 01 13 44.9+24 35 014.65 K0III 5.27.9D:B CPM, 9.11V, +0.92(B-V), +0.25(U-B).,SB:ADS 995A.
HR 361ζ86BD+06 17473441097391033996 A01 13 43.9+07 34 315.24 A7IV 0.10.1D:CPM with HR 362 at 24". ADS 996A is close occultation double, 6.3, 6.3v, 0.05":. Component B, HR 362 is SB; C, 12.2 is,D:1" from B.,DYN:0.012".,SB:ADS 996A, RV var. by 45k/s.
HR 362ζ86BD+06 1757345109740996 B442 01 13 45.3+07 34 426.30 F7V 0.10.1D:CPM with HR 361.,DYN:0.012".,SB:ADS 996B, 6.7, 8.7v, sep. 0.001", 9.0750d, K 51.1k/s, V0 +10.4k/s, asini 6.37.
HR 363BD+27 196735174576I 444 01 14 05.0+28 31 476.43 S3+/2- G:Sigma Pup group.,S:Also classified S3 Zr1 Ti3.,VAR:SRb?, amp. 0.15V.
HR 36487BD+15 1777374923262083 445 01 14 07.6+16 08 015.98 B8III S:HgMn star.,VAR:Alpha CV?, 5.94 - 5.98V.
HR 36788BD+06 1817446109753 01 14 42.4+06 59 436.03 gG6
HR 371BD+32 223757854567I 01 16 18.8+33 06 536.02 K1III C:IR source in this approximate position corresponds to a Seyfert galaxy.
HR 374BD+30 196772454580 01 17 24.1+31 44 416.73 R K0
HR 37889BD+02 18578041097931034 01 17 48.0+03 36 525.16 A3V G:Ursa cluster? UMa stream. Possible Eggen group, with HR 63, q.v.
HR 383υ90BD+26 22079647463745 01 19 28.0+27 15 514.76 A3V
HR 38991BD+27 2158126746472089I 01 21 07.4+28 44 175.23 gK5
HR 397BD+19 226838874682I 01 23 24.9+20 28 085.97 K5
HR 407BD+22 2268634747072096 01 25 35.7+23 30 426.18 F5III SB:5.4291d, K 14.5k/s, V0 -15.9k/s, asini 1.00.
HR 413ρ93BD+18 187872392436 506 01 26 15.3+19 10 205.38 F2V: v
HR 41494BD+18 1898763924441039 01 26 41.7+19 14 255.50 K1III G:Wolf 630 group.
HR 419BD+02 21188031098951148 01 26 53.5+03 32 076.58 B9V+A8V 2.56.0D:Binary. Companion 9.38V, +0.19(B-V), +0.00(U-B), A8V, vsini 48k/s.,DYN:0.016".
HR 426BD+07 2138949109907W 519 01 28 22.9+07 57 416.20 K1III 2.169.0D:CPM. Component B is BD+7d214, 8.02V, +0.53(B-V), +0.06(U-B), G0.
HR 43297BD+17 210910092463 VX Psc01 29 52.9+18 21 206.02 A4IV VAR:Delta Sct 5.90 - 5.92V, 0.131d.
HR 434μ98BD+05 19491381099262099IW 01 30 11.1+06 08 384.84 K4III 5.6182.5R:Diam. 0.0030".
HR 437η99BD+14 23192709248450I1199 532 01 31 29.0+15 20 453.62 G7IIIa 3.60.8D:CPM.,DYN:0.003".,VAR:ADS 1199B, 8.0 - 11.5v?
HR 450BD+17 224964092520I 01 34 49.1+18 27 385.89 M2IIIab
HR 455101BD+13 240976692530 559 01 35 46.4+14 39 416.22 B9.5III
HR 457BD+16 176978092531 01 35 54.8+17 26 015.80 R F0IV
HR 463π102BD+11 2059919925361046 01 37 05.9+12 08 305.57 F0V
HR 475105BD+15 2451016492558 01 39 40.8+16 24 215.97 K2III
HR 484BD+25 276103087487021151326 01 41 18.4+25 44 456.17 F2III 4.410.6D:AB CPM; B is F2III; C optical.,SB:ADS 1326A, 4.4347d, K 81.5k/s, V0 +4.6k/s, msin3i 1.16, asini 4.94.
HR 489ν106BD+04 2931038011006556I 01 41 25.9+05 29 154.44 K3IIIbBa0.1
HR 493107BD+19 2791047674883W 600 01 42 29.8+20 16 075.24 K1V 6.419.0
HR 508109BD+19 2821069792611I 01 44 55.8+20 04 596.27 G3Va
HR 510ο110BD+08 2731076111011060I 615 01 45 23.6+09 09 284.26 G8III N:Torcularis Septentrionalis.
HR 515BD+16 1961084592622 VY Psc01 46 35.3+17 24 476.55 A9III VAR:Delta Sct 6.54 - 6.59V, about 0.2d.
HR 527BD+02 270110371101382121 01 48 26.0+03 41 085.91 G9III
HR 549ξ111BD+02 2901155911020665I 654 01 53 33.3+03 11 154.62 K0III SB:1672.4d, K 4.64k/s, V0 +29.51k/s, asini 105.
HR 582112BD+02 31112235110266 691 02 00 09.2+03 05 505.88 G2IV
HR 595α113BD+02 3171244601615 B02 02 02.8+02 45 495.23 H A3m 1.02.0D:Binary with HR 596, q.v.,DYN:0.017".,VAR:Alpha CV?
HR 596α113BD+02 317124471102911615 A705 02 02 02.8+02 45 494.33 H A0pSiSr 1.04.0D:4.18 A2p, 5.21 Am, 933.05y, a = 4.0". Colors for combined light. Combined mag. 3.82V.,DYN:0.017".,N:Alrisha; Alrischa; Alrescha; El Rischa; Al Richa; Rescha; Okda; Kaitain.,VAR:Alpha CV?, 3.79 - 3.83V. Although the NSV identifies the variable as HR 596, the magnitudes given are for the blend of,VAR:HR 595/6; uncertain which component is the variable.
HR 614BD+07 32412872110337I WZ Psc02 06 12.3+08 14 516.31 M2III: R:Diam. 0.0022".,VAR:SR 6.20 - 6.38V, about 20d.
HR 87151BD+00 4939216701127836 22 54 59.5+01 03 536.11 A7III
HR 8730BD+03 47992170191278603834 22 57 32.8+03 48 376.28 K1III
HR 8734BD-03 55392171071464123836D 22 58 15.5-02 23 436.16 G8IV 1.30.0D:Sep. 0.02", but duplicity uncertain. Unresolved by speckle interferometry.
HR 8735BD-02 5858217131146415 22 58 23.7-01 24 376.37 F0-2V G:Hyades moving group.
HR 8738BD+06 5092217186127874 22 58 42.6+07 20 236.33 A1V
HR 87422BD+00 495021726412788116431 22 59 27.4+00 57 465.43 gK1 7.73.9
HR 87503BD-00 44432174281464433840 Var?23 00 37.9+00 11 096.21 G4III VAR:Amp. 0.018V, pulsating.
HR 8751BD+02 4594217459127894I 23 00 42.9+03 00 425.83 K4III G:Wolf 630 group.
HR 8773β4BD+03 48182178911279341602 1441023 03 52.6+03 49 124.53 B6Ve vN:Fum al Samakah.,S:Width of H alpha varies slightly. Rotationally unstable shell star.
HR 8776BD+05 5123217926127937 23 04 01.0+06 37 006.41 F2V
HR 8785BD+00 4963218103127960 23 05 17.6+01 18 256.39 G9III
HR 88075BD+01 46862185271279933854 23 08 40.9+02 07 405.40 G8III-IV
HR 8852γ6BD+02 4648219615128085878I 23 17 09.9+03 16 563.69 G9-III:Fe-2 M:High space velocity?
HR 88787BD+04 49972200091281263871I 23 20 20.6+05 22 535.05 K2III
HR 8897BD-00 4509220406128156IW 23 23 31.9+00 17 296.31 K2 4.041.7
HR 8911κ8BD+00 4998220825128186884W Kap Psc23 26 56.0+01 15 204.94 A0pCrSi:Sr: v7.0163.4D:AB optical. Component A suspected occultation double.,G:Member of Pleiades group.,S:Oxygen deficient relative to magnesium. Many uranium lines; possibly the uncommon element holmium. Uranium and osmium,S:may be due to supernova explosion in a nearby star.,VAR:Alpha CV 4.91 - 4.96V, 0.58525:d. Period changes? Magnetic and spectrum variable, 0.5805d.
HR 89129BD+00 4999220858128188W 1456823 27 14.8+01 07 216.25 G7III D:Probably single star.
HR 8916θ10BD+05 51732209541281961614I 23 27 58.1+06 22 444.28 K1III
HR 893413BD-01 4450221409146756 23 31 57.6-01 05 096.38 K1III
HR 894414BD-02 59862216751467803890 23 34 09.0-01 14 515.87 A2m G:Hyades group.
HR 895416BD+01 47442219501282813895D 23 36 23.3+02 06 085.68 F6Vb vw 0.10.0D:Duplicity questionable.,SB:6.3, 6.4v, sep. 0.011", 45.459d, K 40.10k/s, V0 +48.43k/s, msin3i 3.49, asini 23.29.
HR 8969ι17BD+04 5035222368128310892IW 1465723 39 57.0+05 37 354.13 F7V 8.769.9D:Optical.
HR 8983BD+06 5183222602128335 1467223 41 56.7+07 15 025.89 A3Vn VAR:Delta Sct?
HR 8984λ18BD+00 50372226031283361620 23 42 02.8+01 46 484.50 A7V G:Sirius group; UMa stream.
HR 900419BD+02 47092230751283743908I TX Psc23 46 23.5+03 29 125.04 C5II G:Gamma Leo group.,R:Occultation diam. = 0.0080 - 0.0102".,S:Technetium found in spectrum.,VAR:Lb 6.9 - 7.7p.
HR 901220BD-03 57072232521469151623W 23 47 56.5-02 45 425.49 G8III 4.4172.7G:Hyades group.
HR 9015BD+01 4773223346128393 23 48 49.3+02 12 516.46 F5III-IV
HR 902221BD+00 5054223438128401 23 49 27.5+01 04 345.77 A5Vm
HR 903322BD+02 47252237191284273918I 23 51 57.9+02 55 495.55 K4IIIaBa0.3 R:Occultation diam. <0.002".
HR 904124BD-03 5723223825146954W 23 52 55.6-03 09 205.93 G9III 0.00.1D:Sep. 0.107".
HR 904225BD+01 4792223855128436 23 53 04.8+02 05 266.28 A1V
HR 9047BD-00 45852240621469733920I XZ Psc23 54 46.6+00 06 335.61 M5III R:Diam. 0.0067".,VAR:Lb 5.55 - 5.97V.
HR 904826BD+06 5216224103128466 23 55 07.8+07 04 166.21 B9V
HR 906727BD-04 5996224533147008900I17137 1478523 58 40.4-03 33 224.86 G9III 5.31.1DYN:0.007".,VAR:ADS 17137B, 9.0 - 11.5V.
HR 9072ω28BD+06 5227224617128513902I 1479323 59 18.7+06 51 484.01 F4IV 2.21.0SB:F2, F6 2.158d, K 6.5Vk/s, V0 -6.0Vk/s, asini 0.181. Possibly triple system: SB, 4.3, 6.5v, sep. 0.00002", and,SB:6.5 at 1.0".
HR 908729BD-03 5749224926147041 1480400 01 49.4-03 01 395.10 B7III-IV S:Sp. shows Mn.
HR 908930BD-06 63452249351470421630I YY Psc00 01 57.6-06 00 514.41 M3III eS:Ultraviolet FeII emission.,VAR:Lb? 4.35 - 4.41V.
HR 909231BD+08 5164224995128544 00 02 24.2+08 57 256.32 A6V
HR 909332BD+07 51212250031285473933 00 02 29.7+08 29 085.63 F0V C:Other UBV data: 5.68 to 5.78V with one discordant 5.32V; +0.31 to +0.42(B-V) with one discordant +0.19(B-V); -0.02 to,C:+0.01(U-B) with one discordant +0.13(U-B).

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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