Kataloge

Pisces / 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 2 BD-01 4525 6 128569 00 05 03.8 -00 30 11 6.29 gG9
HR 3 33 BD-06 6357 28 128572 1002 I Var? 00 05 20.1 -05 42 27 4.61 K0IIIbCN-0.5 2.5 0.0 SB: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 11 BD-03 2 315 128595 Var? 00 07 44.1 -02 32 56 6.43 B8IIIpSi N:4 Cet in Psc.
HR 14 BD-03 3 352 128602 2006 I AP Psc 00 08 12.1 -02 26 52 6.07 K2III+F 2.0 0.0 D: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 26 34 BD+10 8 560 91750 122 00 10 02.3 +11 08 44 5.51 B9Vn e 4.4 7.7 D:Companion 9.44V, +0.34(B-V), -0.14(U-B), G5Ve.,S:H and K lines in emission, lithium strong.
HR 29 BD-06 11 587 128621 D 00 10 18.8 -05 14 55 5.84 K1III D:Suspected occultation double.
HR 50 35 BD+08 19 1061 109087 191 UU Psc 00 14 58.8 +08 49 15 5.79 F0IV 0.0 0.0 D: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 59 36 BD+07 27 1227 109100 2015 00 16 34.1 +08 14 24 6.11 G8II-III
HR 67 BD+00 28 1367 109119 2017 00 17 47.7 +01 41 20 6.17 K0II
HR 69 BD+10 25 1419 91832 00 18 17.2 +11 12 21 6.05 K0III
HR 80 41 BD+07 36 1635 109152 1008 I 132 00 20 35.9 +08 11 25 5.37 gK3
HR 81 BD+10 32 1663 91858 287 00 20 54.5 +10 58 37 6.56 A0V 0.2 0.6 D:B9.5, A2.
HR 86 42 BD+12 25 1796 91866 2020 303 00 22 25.5 +13 28 57 6.23 K3III 4.6 28.9 D:Optical.
HR 94 BD-03 49 2023 128743 2021 00 24 29.7 -02 13 09 6.07 K1III
HR 97 44 BD+01 57 2114 109192 1010 W 00 25 24.2 +01 56 23 5.77 G5III D:Suspected double probably single.,G:Sirius group?
HR 103 47 BD+17 55 2411 91910 I TV Psc 00 28 02.9 +17 53 35 5.06 M3III v G:Zeta Her group; Hyades group.,VAR:SR 4.65 - 5.42V, 49d, replaced by cycles 70 - 85d.
HR 106 48 BD+15 63 2436 91912 1012 I 00 28 12.7 +16 26 42 6.06 K5III
HR 107 BD+09 47 2454 109224 2028 00 28 20.1 +10 11 23 6.04 F6Va vw G:Wolf 630 group.
HR 131 52 BD+19 79 2910 74084 2033 452 00 32 35.5 +20 17 40 5.38 K0III 6.8 49.6
HR 132 51 BD+06 64 2913 109262 2032 449 Var? 00 32 23.8 +06 57 20 5.67 B9.5V 0.7 0.0 D: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 141 BD+12 57 3166 91980 00 34 55.3 +13 22 16 6.40 K0
HR 145 BD+12 59 3268 91990 00 35 54.7 +13 12 24 6.41 F7V
HR 155 53 BD+14 76 3379 91995 2039 AG Psc 00 36 47.3 +15 13 54 5.89 B2.5IV v VAR: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 161 BD+02 80 3457 109315 2040 00 37 30.5 +03 08 07 6.39 K4III G:Sigma Pup group.
HR 166 54 BD+20 85 3651 74175 W 245 00 39 21.8 +21 15 02 5.87 K0+V 4.9 122.0 VAR:5.83 - 5.89V.
HR 167 55 BD+20 87 3690 74182 I 558 00 39 55.6 +21 26 18 5.36 K0III+F3V 3.2 6.6 D:Binary.,DYN:0.007".
HR 211 57 BD+14 111 4408 92072 I 293 00 46 33.0 +15 28 32 5.38 M4IIIa VAR:Lb?, 5.32 - 5.45V.
HR 213 58 BD+11 96 4482 92080 2050 00 47 01.5 +11 58 26 5.50 G8II
HR 214 59 BD+18 101 4490 92082 2051 XX Psc 00 47 13.6 +19 34 44 6.13 F0Vn G:Hyades group.,VAR:Delta Sct? 5.99 - 6.03V, 0.1040d.
HR 216 60 BD+05 104 4526 109461 00 47 23.6 +06 44 27 5.99 G8III
HR 217 61 BD+20 105 4568 74280 00 47 54.8 +20 55 31 6.54 F8V G:Hyades group.
HR 221 62 BD+06 105 4627 109470 00 48 17.4 +07 18 00 5.93 G8III
HR 222 BD+04 123 4628 109471 1019 W 00 48 23.0 +05 16 50 5.75 K2V 4.6 181.2
HR 224 δ 63 BD+06 107 4656 109474 28 I W 00 48 41.0 +07 35 06 4.43 K4IIIb 8.6 113.3 R:Occultation diam. = 0.0042".
HR 225 64 BD+16 76 4676 92099 1020 W 00 48 58.7 +16 56 26 5.07 F8V 7.4 76.7 D: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 230 65 BD+26 131 4757 74295 683 B 00 49 52.8 +27 42 39 7.00 F4III 0.0 4.5 C:Colors for blend with HR 231. Mag. for blend, 5.56V.,D:CPM with HR 231.,DYN:0.004".,G:Hyades group.
HR 231 65 BD+26 131 4758 74296 683 A 00 49 53.2 +27 42 37 7.10 F5III 0.0 4.5 D:CPM with HR 230.,DYN:0.004".,G:Hyades group.
HR 243 BD+02 118 4928 109507 00 51 18.3 +03 23 06 6.37 K0III G:Wolf 630 group.
HR 254 66 BD+18 122 5267 92145 746 00 54 35.2 +19 11 18 5.74 R A1VN 0.8 0.5 D:AB 6.23 A1V, 6.89 A4V, 360.4y, a = 0.700". Combined mag., colors.,DYN:0.011".
HR 259 BD+23 126 5316 74365 I 346 00 55 14.7 +24 33 25 6.20 M4IIIab
HR 262 67 BD+26 151 5382 74373 2059 00 55 58.5 +27 12 34 6.09 A5IV
HR 274 68 BD+28 157 5575 74395 1023 I 00 57 50.2 +28 59 32 5.42 gG6
HR 276 BD+12 119 5612 92183 00 57 54.5 +13 41 45 6.32 G8III G:UMa stream.
HR 277 BD+20 131 5641 74402 805 00 58 18.9 +21 24 16 6.37 R A2V 1.4 0.4 D:ADS 805, 790y.
HR 284 BD+05 131 5820 109581 I W WW Psc 00 59 49.7 +06 28 59 6.11 M2III 7.1 31.0 VAR:Lb 5.95 - 6.12V.
HR 291 σ 69 BD+31 168 6118 54374 01 02 49.1 +31 48 16 5.50 B9.5V SB:81.12d, K 54.3k/s, V0 +10.4k/s, msin3i 0.547, asini 26.4.
HR 294 ε 71 BD+07 153 6186 109627 36 I D 01 02 56.6 +07 53 24 4.28 K0III 0.0 0.2 D:Suspected occultation double, 5.2, 5.2v, sep. 0.25".
HR 303 BD+28 174 6301 74471 01 04 27.6 +29 39 31 6.19 F7IV-V
HR 307 73 BD+04 172 6386 109656 I 01 04 52.6 +05 39 23 6.00 gK5
HR 308 72 BD+14 163 6397 92230 1028 889 01 05 05.4 +14 56 46 5.68 F4II-III 7.4 55.2 D:Visual pair optical.,S:Luminosity variously classified as II, III, V.,SB:ADS 889A.
HR 310 ψ1 74 BD+20 156 6456 74482 899 A 397 01 05 40.9 +21 28 24 5.34 A1Vn 0.3 29.9 D:CPM with HR 311. Third component optical.
HR 311 ψ1 74 BD+20 157 6457 74483 899 B 01 05 41.7 +21 27 55 5.56 A0Vn 0.3 29.9 D:CPM with HR 310.
HR 313 77 BD+04 175 6479 109666 903 A 01 05 49.2 +04 54 30 6.35 F3V 1.0 33.0 D:CPM with HR 314. Faint companions probably optical.,G:Wolf 630 group.
HR 314 77 BD+04 176 6480 109667 903 B 01 05 51.4 +04 54 34 7.25 F6V 1.0 33.0 D:CPM with HR 313.,G:Wolf 630 group.
HR 319 75 BD+12 135 6557 92250 2068 01 06 33.6 +12 57 22 6.12 G8III
HR 327 78 BD+31 185 6680 54445 2072 01 08 01.3 +32 00 44 6.25 F5IV G:Hyades moving group.
HR 328 ψ2 79 BD+19 185 6695 74506 01 07 57.2 +20 44 21 5.55 A3V
HR 330 80 BD+04 190 6763 109697 2073 W 410 01 08 22.2 +05 38 59 5.52 F0III-IV 3.8 159.3 D:Companions probably optical.,G:UMa stream.,VAR:Delta Sct?
HR 339 ψ3 81 BD+18 153 6903 92283 Var? 01 09 49.2 +19 39 31 5.55 G0III
HR 341 BD+24 186 6953 74530 I 01 10 19.4 +25 27 28 5.80 K7III
HR 344 BD+14 175 6966 92288 I 01 10 11.5 +15 40 27 6.06 M0III
HR 349 82 BD+30 181 7034 54493 01 11 06.8 +31 25 29 5.16 F0V
HR 351 χ 84 BD+20 172 7087 74544 1032 I 01 11 27.2 +21 02 05 4.66 G8.5III-IIIa
HR 352 τ 83 BD+29 190 7106 74546 43 I 01 11 39.6 +30 05 23 4.51 K0.5IIIb
HR 356 BD+29 195 7229 74561 990 01 12 59.5 +30 03 51 6.19 G9III+G1V 4.1 10.8 D:AB CPM. Component B, 10.25V, +0.79(B-V), +0.29(U-B), G1V.
HR 360 φ 85 BD+23 158 7318 74571 2082 I 995 01 13 44.9 +24 35 01 4.65 K0III 5.2 7.9 D:B CPM, 9.11V, +0.92(B-V), +0.25(U-B).,SB:ADS 995A.
HR 361 ζ 86 BD+06 174 7344 109739 1033 996 A 01 13 43.9 +07 34 31 5.24 A7IV 0.1 0.1 D: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 362 ζ 86 BD+06 175 7345 109740 996 B 442 01 13 45.3 +07 34 42 6.30 F7V 0.1 0.1 D: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 363 BD+27 196 7351 74576 I 444 01 14 05.0 +28 31 47 6.43 S3+/2- G:Sigma Pup group.,S:Also classified S3 Zr1 Ti3.,VAR:SRb?, amp. 0.15V.
HR 364 87 BD+15 177 7374 92326 2083 445 01 14 07.6 +16 08 01 5.98 B8III S:HgMn star.,VAR:Alpha CV?, 5.94 - 5.98V.
HR 367 88 BD+06 181 7446 109753 01 14 42.4 +06 59 43 6.03 gG6
HR 371 BD+32 223 7578 54567 I 01 16 18.8 +33 06 53 6.02 K1III C:IR source in this approximate position corresponds to a Seyfert galaxy.
HR 374 BD+30 196 7724 54580 01 17 24.1 +31 44 41 6.73 R K0
HR 378 89 BD+02 185 7804 109793 1034 01 17 48.0 +03 36 52 5.16 A3V G:Ursa cluster? UMa stream. Possible Eggen group, with HR 63, q.v.
HR 383 υ 90 BD+26 220 7964 74637 45 01 19 28.0 +27 15 51 4.76 A3V
HR 389 91 BD+27 215 8126 74647 2089 I 01 21 07.4 +28 44 17 5.23 gK5
HR 397 BD+19 226 8388 74682 I 01 23 24.9 +20 28 08 5.97 K5
HR 407 BD+22 226 8634 74707 2096 01 25 35.7 +23 30 42 6.18 F5III SB:5.4291d, K 14.5k/s, V0 -15.9k/s, asini 1.00.
HR 413 ρ 93 BD+18 187 8723 92436 506 01 26 15.3 +19 10 20 5.38 F2V: v
HR 414 94 BD+18 189 8763 92444 1039 01 26 41.7 +19 14 25 5.50 K1III G:Wolf 630 group.
HR 419 BD+02 211 8803 109895 1148 01 26 53.5 +03 32 07 6.58 B9V+A8V 2.5 6.0 D:Binary. Companion 9.38V, +0.19(B-V), +0.00(U-B), A8V, vsini 48k/s.,DYN:0.016".
HR 426 BD+07 213 8949 109907 W 519 01 28 22.9 +07 57 41 6.20 K1III 2.1 69.0 D:CPM. Component B is BD+7d214, 8.02V, +0.53(B-V), +0.06(U-B), G0.
HR 432 97 BD+17 210 9100 92463 VX Psc 01 29 52.9 +18 21 20 6.02 A4IV VAR:Delta Sct 5.90 - 5.92V, 0.131d.
HR 434 μ 98 BD+05 194 9138 109926 2099 I W 01 30 11.1 +06 08 38 4.84 K4III 5.6 182.5 R:Diam. 0.0030".
HR 437 η 99 BD+14 231 9270 92484 50 I 1199 532 01 31 29.0 +15 20 45 3.62 G7IIIa 3.6 0.8 D:CPM.,DYN:0.003".,VAR:ADS 1199B, 8.0 - 11.5v?
HR 450 BD+17 224 9640 92520 I 01 34 49.1 +18 27 38 5.89 M2IIIab
HR 455 101 BD+13 240 9766 92530 559 01 35 46.4 +14 39 41 6.22 B9.5III
HR 457 BD+16 176 9780 92531 01 35 54.8 +17 26 01 5.80 R F0IV
HR 463 π 102 BD+11 205 9919 92536 1046 01 37 05.9 +12 08 30 5.57 F0V
HR 475 105 BD+15 245 10164 92558 01 39 40.8 +16 24 21 5.97 K2III
HR 484 BD+25 276 10308 74870 2115 1326 01 41 18.4 +25 44 45 6.17 F2III 4.4 10.6 D: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 489 ν 106 BD+04 293 10380 110065 56 I 01 41 25.9 +05 29 15 4.44 K3IIIbBa0.1
HR 493 107 BD+19 279 10476 74883 W 600 01 42 29.8 +20 16 07 5.24 K1V 6.4 19.0
HR 508 109 BD+19 282 10697 92611 I 01 44 55.8 +20 04 59 6.27 G3Va
HR 510 ο 110 BD+08 273 10761 110110 60 I 615 01 45 23.6 +09 09 28 4.26 G8III N:Torcularis Septentrionalis.
HR 515 BD+16 196 10845 92622 VY Psc 01 46 35.3 +17 24 47 6.55 A9III VAR:Delta Sct 6.54 - 6.59V, about 0.2d.
HR 527 BD+02 270 11037 110138 2121 01 48 26.0 +03 41 08 5.91 G9III
HR 549 ξ 111 BD+02 290 11559 110206 65 I 654 01 53 33.3 +03 11 15 4.62 K0III SB:1672.4d, K 4.64k/s, V0 +29.51k/s, asini 105.
HR 582 112 BD+02 311 12235 110266 691 02 00 09.2 +03 05 50 5.88 G2IV
HR 595 α 113 BD+02 317 12446 0 1615 B 02 02 02.8 +02 45 49 5.23 H A3m 1.0 2.0 D:Binary with HR 596, q.v.,DYN:0.017".,VAR:Alpha CV?
HR 596 α 113 BD+02 317 12447 110291 1615 A 705 02 02 02.8 +02 45 49 4.33 H A0pSiSr 1.0 4.0 D: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 614 BD+07 324 12872 110337 I WZ Psc 02 06 12.3 +08 14 51 6.31 M2III: R:Diam. 0.0022".,VAR:SR 6.20 - 6.38V, about 20d.
HR 8715 1 BD+00 4939 216701 127836 22 54 59.5 +01 03 53 6.11 A7III
HR 8730 BD+03 4799 217019 127860 3834 22 57 32.8 +03 48 37 6.28 K1III
HR 8734 BD-03 5539 217107 146412 3836 D 22 58 15.5 -02 23 43 6.16 G8IV 1.3 0.0 D:Sep. 0.02", but duplicity uncertain. Unresolved by speckle interferometry.
HR 8735 BD-02 5858 217131 146415 22 58 23.7 -01 24 37 6.37 F0-2V G:Hyades moving group.
HR 8738 BD+06 5092 217186 127874 22 58 42.6 +07 20 23 6.33 A1V
HR 8742 2 BD+00 4950 217264 127881 16431 22 59 27.4 +00 57 46 5.43 gK1 7.7 3.9
HR 8750 3 BD-00 4443 217428 146443 3840 Var? 23 00 37.9 +00 11 09 6.21 G4III VAR:Amp. 0.018V, pulsating.
HR 8751 BD+02 4594 217459 127894 I 23 00 42.9 +03 00 42 5.83 K4III G:Wolf 630 group.
HR 8773 β 4 BD+03 4818 217891 127934 1602 14410 23 03 52.6 +03 49 12 4.53 B6Ve v N:Fum al Samakah.,S:Width of H alpha varies slightly. Rotationally unstable shell star.
HR 8776 BD+05 5123 217926 127937 23 04 01.0 +06 37 00 6.41 F2V
HR 8785 BD+00 4963 218103 127960 23 05 17.6 +01 18 25 6.39 G9III
HR 8807 5 BD+01 4686 218527 127993 3854 23 08 40.9 +02 07 40 5.40 G8III-IV
HR 8852 γ 6 BD+02 4648 219615 128085 878 I 23 17 09.9 +03 16 56 3.69 G9-III:Fe-2 M:High space velocity?
HR 8878 7 BD+04 4997 220009 128126 3871 I 23 20 20.6 +05 22 53 5.05 K2III
HR 8897 BD-00 4509 220406 128156 I W 23 23 31.9 +00 17 29 6.31 K2 4.0 41.7
HR 8911 κ 8 BD+00 4998 220825 128186 884 W Kap Psc 23 26 56.0 +01 15 20 4.94 A0pCrSi:Sr: v 7.0 163.4 D: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 8912 9 BD+00 4999 220858 128188 W 14568 23 27 14.8 +01 07 21 6.25 G7III D:Probably single star.
HR 8916 θ 10 BD+05 5173 220954 128196 1614 I 23 27 58.1 +06 22 44 4.28 K1III
HR 8934 13 BD-01 4450 221409 146756 23 31 57.6 -01 05 09 6.38 K1III
HR 8944 14 BD-02 5986 221675 146780 3890 23 34 09.0 -01 14 51 5.87 A2m G:Hyades group.
HR 8954 16 BD+01 4744 221950 128281 3895 D 23 36 23.3 +02 06 08 5.68 F6Vb vw 0.1 0.0 D: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 8969 ι 17 BD+04 5035 222368 128310 892 I W 14657 23 39 57.0 +05 37 35 4.13 F7V 8.7 69.9 D:Optical.
HR 8983 BD+06 5183 222602 128335 14672 23 41 56.7 +07 15 02 5.89 A3Vn VAR:Delta Sct?
HR 8984 λ 18 BD+00 5037 222603 128336 1620 23 42 02.8 +01 46 48 4.50 A7V G:Sirius group; UMa stream.
HR 9004 19 BD+02 4709 223075 128374 3908 I TX Psc 23 46 23.5 +03 29 12 5.04 C5II G:Gamma Leo group.,R:Occultation diam. = 0.0080 - 0.0102".,S:Technetium found in spectrum.,VAR:Lb 6.9 - 7.7p.
HR 9012 20 BD-03 5707 223252 146915 1623 W 23 47 56.5 -02 45 42 5.49 G8III 4.4 172.7 G:Hyades group.
HR 9015 BD+01 4773 223346 128393 23 48 49.3 +02 12 51 6.46 F5III-IV
HR 9022 21 BD+00 5054 223438 128401 23 49 27.5 +01 04 34 5.77 A5Vm
HR 9033 22 BD+02 4725 223719 128427 3918 I 23 51 57.9 +02 55 49 5.55 K4IIIaBa0.3 R:Occultation diam. <0.002".
HR 9041 24 BD-03 5723 223825 146954 W 23 52 55.6 -03 09 20 5.93 G9III 0.0 0.1 D:Sep. 0.107".
HR 9042 25 BD+01 4792 223855 128436 23 53 04.8 +02 05 26 6.28 A1V
HR 9047 BD-00 4585 224062 146973 3920 I XZ Psc 23 54 46.6 +00 06 33 5.61 M5III R:Diam. 0.0067".,VAR:Lb 5.55 - 5.97V.
HR 9048 26 BD+06 5216 224103 128466 23 55 07.8 +07 04 16 6.21 B9V
HR 9067 27 BD-04 5996 224533 147008 900 I 17137 14785 23 58 40.4 -03 33 22 4.86 G9III 5.3 1.1 DYN:0.007".,VAR:ADS 17137B, 9.0 - 11.5V.
HR 9072 ω 28 BD+06 5227 224617 128513 902 I 14793 23 59 18.7 +06 51 48 4.01 F4IV 2.2 1.0 SB: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 9087 29 BD-03 5749 224926 147041 14804 00 01 49.4 -03 01 39 5.10 B7III-IV S:Sp. shows Mn.
HR 9089 30 BD-06 6345 224935 147042 1630 I YY Psc 00 01 57.6 -06 00 51 4.41 M3III e S:Ultraviolet FeII emission.,VAR:Lb? 4.35 - 4.41V.
HR 9092 31 BD+08 5164 224995 128544 00 02 24.2 +08 57 25 6.32 A6V
HR 9093 32 BD+07 5121 225003 128547 3933 00 02 29.7 +08 29 08 5.63 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).

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)

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