Kataloge

Vela / Yale Bright Star Catalog (HR)

«Yale Bright Star Catalogue, 5th Revised Ed.» Hoffleit D., Warren Jr W.H., 1991 [154]
HR B DM HD SAO FK5 IR M* ADS VarID RA Dec vMag spType dMag Sep Remarks
HR 3178 CD-50 3138 67249 235730 2626 08 04 42.4 -50 35 26 5.95 G5II
HR 3179 CD-46 3764 67341 219400 08 05 20.4 -46 58 44 6.19 B3Vnp
HR 3187 CD-44 4051 67582 219422 3905 08 06 40.4 -45 15 59 5.05 K3III VAR:6.70 - 6.80p.
HR 3203 CD-48 3516 68161 219493 08 09 09.6 -48 41 04 5.70 B8Ib-II
HR 3204 CD-43 3998 68217 219502 2634 Var? 08 09 35.9 -44 07 22 5.21 B2IV-V
HR 3206 γ1 CD-46 3846 68243 219501 W B 3930 08 09 29.3 -47 20 45 4.27 B1IV 2.3 41.2 D:Component B of 5 stars within 2' of HR 3207.,G:Gamma Velorum group.,SB:1.482575d, K 45.0k/s, V0 +9.7k/s, asini 0.916.
HR 3207 γ2 CD-46 3847 68273 219504 309 W A Gam2 Vel 08 09 32.0 -47 20 12 1.78 WC8+O9I v 2.3 41.2 D:See HR 3206. Mag. and colors blended with other companions. C = CoD -46d3848, 7.65V, B6V at 63", physical. D, 9.07V,,D:Am at 94", SB, over 7d?, optical.,G:Gamma Velorum group which includes HR 3206, probably also HD 68157 at 20' and HR 3213 at 36' from A; HII region.,M:Low degree of polarization indicates symmetric shell. The brightest O-type star and one of only four WR stars bright,M:enough to have been observed spectroscopically in UV by COPERNICUS. With 3165, appears capable of producing most of the,M:observed ionization of Gum Neb. The brightest and presumably the nearest Wolf-Rayet binary. Radio emission interpreted,M:as coming from circumstellar gas cloud extending farther than the orbital radius of the binary.,N:Suhail al Muhlif; Al Suhail al Muhlif; "Spectral Gem of Southern Skies".,R:Diam. = 0.00043 - 0.00044".,S:Magnesium and iron depleted by factor of 100 relative to the sun. UV spectrum dominated by supergiant companions. The,S:Wolf-Rayet component appears to be the most massive known. Radio emission indicates a circumstellar gas cloud extending,S:beyond the orbit of the binary. Also classified WC8+O7.5e.,SB:Comp. A of visual double, 78.5d, K 43.1k/s, V0 -18.0k/s, asini 45.8. Alternate orbit 78.5002d, K 70k/s,,SB:V0 +12k/s, msin3i 32, asini 67. Possible mass transfer from WR to O-type component.,VAR:1.6 - 1.8V, 154 sec. Sp. var. in about 200 sec. Variability too great to be explained by the 78.5d SB companion.,VAR:Possibly a third close companion: a collapsed star of less than 2 solar masses.
HR 3213 CD-47 3653 68324 219515 IS Vel 08 09 43.2 -47 56 15 5.23 B1IVe RV:Amp. about 20k/s. Period probably same as for light curve.,VAR:BetaC, Amp. 0.018u, 0.108d.
HR 3227 CD-48 3576 68657 219565 08 11 11.1 -48 27 43 5.82 B3V
HR 3232 CD-46 3902 68808 219587 AH Vel 08 12 00.0 -46 38 39 5.76 F7Ib-II VAR:Cep 5.50 - 5.86V, 4.22717d. Per. and form of light curve vary.
HR 3234 CD-45 3892 68895 219602 W 08 12 30.9 -46 15 51 6.03 B5V 0.8 0.4
HR 3244 CD-46 3929 69144 219629 W Var 08 13 36.2 -46 59 31 5.13 B2.5IV 3.9 35. D:Companion K5V, RV +7k/s, optical.,VAR:Amp. 0.03b.
HR 3247 CD-49 3430 69194 235819 3957 08 13 34.1 -50 11 46 5.51 M1III G:Praesepe cluster.
HR 3250 CD-45 3914 69302 219657 W 08 14 23.9 -45 50 04 5.83 B2IV-V 1.5 0.4
HR 3256 CD-50 3227 69596 235838 08 15 23.3 -50 26 58 6.44 K3-4III
HR 3294 CD-48 3734 70930 219848 W Var? 08 22 31.6 -48 29 25 4.82 B1V 1.0 0.8
HR 3300 CD-51 2980 71043 235933 08 22 55.2 -52 07 26 5.85 A0V
HR 3330 CD-51 3004 71510 235962 W 08 25 31.0 -51 43 41 5.17 B2Ve 4.2 25.7 D:Component B, CoD-51d3003, 10.2v, B8V, optical. Third component G3V may be physical.,G:See HR 2702.
HR 3341 CP-52 1474 71722 235976 2661 08 26 25.2 -52 48 27 6.05 A0V
HR 3350 CP-52 1484 71935 236002 GU Vel 08 27 36.5 -53 05 19 5.09 A9-F0III-IV S:Also classified F3V.,VAR:Delta Sct amp. 0.015V, 0.07:d.
HR 3356 CD-43 4337 72067 219982 2665 W 4106 08 29 07.6 -44 09 38 5.79 B2Vn t 0.1 0.2 VAR:H alpha emission var.
HR 3358 CD-47 4004 72108 219985 W 08 29 04.7 -47 55 45 5.33 B2IV 0.0 0.2 D:AP, 6.4, 6.4v, sep. 0.176", combined mag., color. Components B, 7.7v at 4" binary with AP, C, 9.3v at 19".,SB:Comp. A of visual double; comp. B +15k/s.
HR 3359 CD-44 4462 72127 219996 W 08 29 27.6 -44 43 30 4.99 B2IV 1.7 4.6 D:Components B2III and B2.5V.
HR 3363 CD-45 4183 72232 220007 08 29 45.6 -46 19 55 5.99 B5III
HR 3371 CD-44 4477 72350 220025 W 08 30 39.2 -44 44 14 6.30 B4IV 4.5 3.2 G:Sco-Cen assoc.
HR 3373 CD-38 4566 72436 199329 W 08 31 24.6 -39 03 51 6.31 B4V 1.8 3.8
HR 3375 CD-47 4048 72485 220039 08 31 10.8 -47 52 00 6.39 B2.5V
HR 3382 CP-53 1729 72650 236055 08 31 29.6 -54 23 39 6.34 K3III
HR 3386 CP-52 1517 72737 236062 W 08 32 04.8 -53 12 44 5.69 K0III+A3 1.0 0.8 D:SKYLAB indicates cool star with hot companion.,S:Also classified G8III + A0/1V.
HR 3388 CD-37 4850 72787 199363 Var? 08 33 19.9 -38 22 16 6.49 B2.5V M:Old disk population runaway star.
HR 3389 CD-38 4610 72832 199370 4137 08 33 38.3 -38 50 56 5.96 B5III VAR:5.8 - 5.89B.
HR 3390 CD-46 4300 72900 220103 08 33 30.4 -46 58 16 6.24 K3III
HR 3399 CD-37 4873 72993 199389 W 4143 08 34 29.3 -37 36 41 6.30 K5III 2.3 1.9 D:Components M1IIIa and G7IIIb.,VAR:Amp. 0.09V.
HR 3404 CD-39 4519 73121 199402 08 35 12.6 -39 58 12 6.47 G1V
HR 3407 CD-49 3646 73155 220138 2674 08 34 43.6 -49 56 39 5.01 K1-2II
HR 3413 CD-50 3417 73340 236110 HV Vel 08 35 52.1 -50 58 12 5.80 B8Si v G:In cluster IC 2391.,VAR:Amp. 0.025y, 2.67d. Spectrum var. same period.
HR 3421 CD-39 4574 73524 199438 08 37 19.9 -40 08 51 6.55 G4IV-V
HR 3426 CD-42 4451 73634 220204 324 08 37 38.7 -42 59 21 4.14 A6II
HR 3435 CP-52 1565 73952 236142 W 08 38 44.9 -53 05 26 6.47 B8Vn 7.5 22.2 G:IC 2391 #8.
HR 3439 CD-39 4653 74067 220252 W 4193 08 40 19.3 -40 15 51 5.20 B9V 3.7 4.4 D:Companion A2V.
HR 3440 CP-53 1796 74071 236151 HW Vel 08 39 23.8 -53 26 23 5.48 B5V G:See HR 2702.,G:IC 2391 #13, probable member of the cluster.,VAR:Amp. 0.02V, 0.26145d. Probable beat phenomena.
HR 3442 CP-52 1579 74146 236157 W 4194 08 39 57.6 -53 03 18 5.19 B4IV 4.4 16.6 D:CPM? Companion F0IV.,G:Sco-Cen assoc.; probable member of open cluster IC 2391 (#16). See HR 2702.,SB:Primary of visual double. 3.1d. RV comp. B +12k/s.,VAR:Component A of double. Ell?, 5.17 - 5.27V.
HR 3444 CD-44 4679 74167 220261 4198 08 40 35.3 -45 11 29 5.71 M0III
HR 3445 CD-46 4438 74180 220265 1226 W 4199 08 40 37.6 -46 38 56 3.84 F3Ia 6.9 37.5 C:U-B values scatter from +0.22 to +0.54.,G:Vel OB1.
HR 3447 CP-52 1583 74195 236164 1227 o Vel 08 40 17.6 -52 55 19 3.62 B3IV G:In cluster IC 2391 #20.,N:Sometimes called omicron Vel, but the letter had originally been "o" (Roman), not omicron.,RV:Expanding circumstellar shell.,SB:3.2 hrs.,VAR:Beta C 3.56 - 3.67V, 0.131977d.
HR 3448 CP-52 1584 74196 236165 4197 08 40 17.4 -53 00 55 5.61 B7Vn G:IC 2391 #21.,S:Helium-weak star.,VAR:Beta C?, 5.56 - 5.62V, amp. 0.01b, 0.388d. Possibly the shortest period known for a He-weak star.
HR 3452 CD-46 4448 74272 220284 08 41 13.1 -47 19 01 4.77 A5II
HR 3453 CD-48 4020 74273 220282 08 41 05.3 -48 55 21 5.90 B1.5V S:Also classified B2III.
HR 3456 CD-44 4704 74371 220300 08 41 56.9 -45 24 39 5.23 B6Iae G:Vel OB1.
HR 3462 CD-47 4251 74455 220313 W HX Vel 08 42 16.0 -48 05 57 5.51 B1.5Vn 1.3 0.3 G:In cluster IC 2395 #1; Sco-Cen assoc.,M:Unusually high-velocity interstellar CaII not associated with galactic rotation, but probably part of Vela supernova,M:remnant associated with Pulsar 0833-45 about 3d away.,VAR:Amp. 0.037b, 0.563d.
HR 3466 CP-52 1605 74535 236202 W BC KT Vel 08 42 18.9 -53 06 00 5.52 B8Si 0.8 76.6 D:Binary with HR 3467. Component C 8.0v at 0.5" from B.,G:IC 2391 #31.,VAR:Alpha CV, 5.49 - 5.56V, 3.376d.
HR 3467 CP-52 1607 74560 236205 W A HY Vel 08 42 25.5 -53 06 50 4.86 B3IV 0.8 76.6 D:See HR 3466.,G:Sco-Cen assoc.; IC 2391 #34, probable member of cluster. See HR 2702.,VAR:Amp. 0.015b, 0.0284d.
HR 3476 CD-49 3761 74753 220361 2689 08 43 40.3 -49 49 22 5.16 B0IIIn
HR 3477 CD-42 4569 74772 220371 W 08 44 24.0 -42 38 57 4.07 G5III 7.1 45.3 G:Possibly member open cluster Trumpler 10.
HR 3485 δ CP-54 1788 74956 236232 W 08 44 42.2 -54 42 30 1.96 A1V 3.0 2.2 D:AB binary with CPM double companion CD at 69". CD 11.0, 13.5v sep. 6".,DYN:0.034".,G:In Ursa cluster? Sirius group?,RV:Two determinations of vsini, 0 and 80k/s.
HR 3487 CD-45 4517 75063 220422 08 46 01.7 -46 02 30 3.91 A1III
HR 3488 CD-40 4602 75081 220432 08 46 23.8 -41 07 32 6.21 B9Ve t VAR:H alpha emission var.
HR 3494 CD-45 4526 75149 220442 08 46 30.6 -45 54 46 5.46 B3Ia D:Wide CPM pair with HR 3496.,G:Sco-Cen assoc.; Vel OB1.
HR 3496 CD-45 4541 75276 220464 08 47 18.9 -46 09 20 5.75 F2Iab C:U-B values scatter from +0.22 to +0.55.,D:See HR 3494.,G:Vel OB1.
HR 3497 CD-41 4507 75289 220481 08 47 40.5 -41 44 14 6.36 G0Ia-0:
HR 3501 CD-41 4516 75387 220495 08 48 08.8 -42 27 50 6.43 B2IV-V G:In open cluster Trumpler 10.
HR 3503 CP-52 1675 75466 236284 08 48 00.2 -52 51 02 6.30 B8V G:IC 2391 #50.,RV:Other determinations as high as +34k/s.
HR 3514 CD-39 4838 75630 220531 08 49 39.2 -40 19 14 5.48 A2/3IV
HR 3517 CD-38 4925 75654 199682 2697 HZ Vel 08 49 52.4 -39 08 30 6.39 A5III VAR:Delta Sct, 0.087d.
HR 3520 CD-44 4861 75710 220540 2698 08 49 47.7 -45 18 29 4.93 A2III
HR 3525 CD-41 4560 75759 220552 08 50 21.0 -42 05 24 6.00 B1-2III G:Sco-Cen assoc.; doubtful member Vel OB1.,S:Also classified O9IV, O9V, B0V, B1IIIn.,SB:33.311d, K 121.3k/s, V0 +23.4k/s, msin3i 18.0, a1sini 43.1, a2sini 53.5. Massive system similar to,SB:Iota Ori; might be eclipsing.
HR 3527 CD-46 4661 75821 220561 W 08 50 33.5 -46 31 45 5.10 B0III 4.1 3.2 D:CPM.,G:Sco-Cen assoc.,RV:High-velocity interstellar CaII not associated with galactic rotation, but probably part of Vela SN remnant associated,RV:with Pulsar 0833-45 about 3d away.
HR 3530 CD-42 4723 75926 220581 08 51 27.9 -42 30 16 6.55 A1Vn
HR 3535 CD-38 4980 76110 199737 08 52 48.0 -38 43 27 5.82 M0III
HR 3539 CD-47 4460 76161 220609 08 52 38.6 -48 21 33 5.91 B3Vn G:Sco-Cen assoc.
HR 3542 CD-51 3303 76230 236362 W 08 52 40.8 -52 07 45 6.39 A0V 1.6 2.8 D:Binary. Combined mag., colors.
HR 3548 CD-39 4924 76304 220628 08 53 50.7 -40 26 51 6.47 K0II-III+A5
HR 3551 CD-47 4480 76360 220636 W 08 53 50.7 -47 31 15 5.33 A9IV-V 0.0 0.1 D:6.1 Am, 6.1, 7.24y, a = 0.1036". Combined mag., color.,DYN:0.017".,SB:9.07d.
HR 3562 CD-44 4951 76566 220664 W IY Vel 08 55 19.3 -45 02 30 6.26 B3IV 6.5 35.0 VAR:Amp. 0.04:V. Multiple periods 1.97, 1.73 and 1.66d found, but subsequently questioned.
HR 3570 CP-54 1925 76653 236405 08 55 11.9 -54 57 56 5.71 F6V
HR 3574 CP-52 1788 76805 236417 W 08 56 19.4 -52 43 25 4.69 B5V 3.0 2.8 SB:0.9147d, K 46.3k/s, V0 +22.2k/s, asini 0.577.
HR 3583 CD-48 4282 77020 220703 08 57 55.8 -48 34 24 5.87 G8-K0II
HR 3588 CD-46 4810 77140 220717 W FZ Vel 08 58 52.3 -47 14 05 5.18 Am 6.0 24.2 G:Hyades moving group.,S:Delta Sct type spectrum.,VAR:Delta Sct 5.15 - 5.17V, 0.065d.
HR 3591 CD-40 4810 77258 220730 1234 4346 09 00 05.4 -41 15 14 4.45 G8-K1III+A S:Also variously classified Fp, F8III.,SB:74.1469d, K 17.8k/s, V0 -7.4k/s, asini 18.1.
HR 3593 CD-42 4875 77320 220738 IU Vel 09 00 22.2 -43 10 24 6.07 B2.5Vn t S:Variable H alpha emission.,VAR:Beta Cep 6.02 - 6.06V, about 7 hrs. with beat phenomenon.
HR 3600 CD-41 4720 77475 220760 IZ Vel 09 01 20.8 -41 51 52 5.55 B5V VAR:Amp. 0.03:V. Multiple periods 9.64, 14.4 and 10.7d.
HR 3602 CD-38 5154 77580 199902 09 02 06.4 -39 24 09 6.27 K1III-IV
HR 3605 CD-51 3430 77653 236518 W 09 01 44.6 -52 11 18 5.23 B9Si 1.2 0.9
HR 3611 CP-53 2072 77907 236542 09 03 05.2 -53 32 59 6.40 B6V
HR 3614 CD-46 4883 78004 220803 342 09 04 09.3 -47 05 52 3.75 K2III
HR 3629 CP-55 1957 78548 236611 09 06 34.0 -55 48 12 6.11 B2IV-V
HR 3631 CD-50 3849 78599 236618 2722 09 07 14.7 -51 12 43 6.73 K4III
HR 3634 λ CD-42 4990 78647 220878 345 I W Lam Vel 09 07 59.8 -43 25 57 2.21 K4.5Ib-II e 12.6 18.2 M:Young disk population.,N:Alsuhail; Al Suhail al Wazn; Suhail.,S:Ultraviolet FeII emission.,VAR:Lc 2.14 - 2.22V.
HR 3647 CD-48 4471 79025 220910 09 09 45.1 -49 25 29 6.48 A9Vn S:Also classified Am.
HR 3654 CD-44 5206 79186 220928 GX Vel 09 11 04.4 -44 52 05 5.00 B5Ia VAR:Amp. 0.07V.
HR 3656 CD-38 5358 79241 200084 09 11 41.0 -39 15 32 6.00 B6V
HR 3658 CD-46 4987 79275 220937 09 11 33.2 -46 35 02 5.79 B2III/IV
HR 3661 CD-43 5041 79416 220952 W KL Vel 09 12 30.6 -43 36 49 5.57 B8Vp:Si: 0.7 2.8 D:AB 6.7, 7.2v sep. 0.11". Combined mag., colors of ABC.
HR 3667 CD-38 5376 79523 200119 4423 09 13 25.9 -38 36 59 6.31 A0V
HR 3668 CD-41 4904 79524 220962 09 13 18.6 -42 16 25 6.29 K2III
HR 3670 CD-46 5010 79621 220965 09 13 34.5 -47 20 19 5.92 B9Ve v S:Variable H alpha.
HR 3672 CD-43 5068 79694 220972 2731 4428 09 14 08.2 -44 08 45 5.85 B5/6IV/V G:Sco-Cen assoc. See HR 2702.
HR 3674 CD-42 5086 79735 220978 W 09 14 24.5 -43 13 39 5.25 B4V 4.1 5.8 G:Sco-Cen assoc. See HR 2702.
HR 3677 CD-37 5578 79807 200152 09 14 57.2 -37 36 09 5.86 G0V
HR 3679 CP-55 2035 79846 236749 2736 4429 09 14 18.0 -55 34 11 5.27 G8II-III VAR:6.3 - 8.1p.
HR 3680 CD-45 4982 79900 220998 W 09 15 14.6 -45 33 20 6.25 B8V 0.9 0.8 D:Binary, combined mag., colors.
HR 3682 CD-38 5408 79917 200159 2737 09 15 36.7 -38 34 12 4.94 K0III
HR 3684 CD-36 5505 79940 200163 W 09 15 45.1 -37 24 48 4.62 F5III 9.8 11.3
HR 3688 CD-44 5305 80057 221010 W 4436 09 16 04.2 -44 53 55 6.04 A1Ib 8.0 6.8 VAR:6.3 - 6.34p.
HR 3692 CD-43 5103 80108 221014 4437 09 16 23.1 -44 15 57 5.12 K3Ib S:Also classified K4III.,VAR:5.08 - 5.14V.
HR 3694 CD-38 5430 80170 200185 09 16 57.2 -39 24 05 5.33 K5III-IV RV:Period 1 - 2 months?
HR 3700 CP-53 2281 80435 236819 09 17 42.3 -54 29 43 6.33 K3III
HR 3703 CD-50 4001 80456 236824 09 18 05.8 -51 03 04 5.26 B7-8III
HR 3708 CD-51 3693 80558 236837 4454 09 18 42.2 -51 33 38 5.87 B6Iae C:B-V values scatter from +0.43 to +0.62, U-B from -0.16 to -0.40.
HR 3716 CD-37 5668 80774 200257 09 20 29.6 -37 34 53 6.05 K3/4III
HR 3717 CP-54 2186 80781 236851 09 19 32.6 -55 11 12 6.28 B5V G:Formerly considered member of Sco-Cen assoc. (probably not member).,M:Close to error box of X-ray source 3U0918-55.
HR 3726 CD-41 5023 81034 221103 09 21 50.9 -42 11 42 5.58 M1III
HR 3729 CD-39 5446 81134 200299 09 22 36.7 -39 46 29 6.54 K1III
HR 3730 CD-45 5099 81136 221109 2746 4473 09 22 24.0 -46 02 51 5.75 G6-8III VAR:5.72 - 5.76V.
HR 3732 CP-54 2213 81157 236887 09 21 50.0 -55 30 54 5.63 A3IV s:
HR 3734 κ CP-54 2219 81188 236891 353 09 22 06.8 -55 00 39 2.50 B2IV-V G:Sco-Cen assoc.,M:Third UHURU Catalogue suggests Kappa Vel as optical counterpart of 3U0918-55, but HR 3717 is much closer.,SB:116.65d, K 46.5k/s, V0 +21.9k/s, asini 73.2.
HR 3735 CD-37 5721 81309 200320 09 23 44.8 -37 45 26 6.48 A1mA5-F0
HR 3737 CD-38 5541 81411 200330 W 09 24 16.3 -39 25 33 6.06 A7V: 0.0 0.1 S:Also classified A6/7III.
HR 3739 CD-51 3767 81471 236930 09 23 59.5 -51 44 14 6.08 A7Iab C:B-V values scatter from +0.49 to +0.66, U-B from +0.06 to +0.39.
HR 3746 CD-39 5507 81780 221167 09 26 28.5 -40 30 07 6.20 A7III
HR 3753 CP-52 2360 81848 236972 09 26 18.1 -53 22 45 5.11 B6V G:Sco-Cen assoc.
HR 3784 CD-50 4204 82419 237042 09 30 05.2 -51 31 02 5.45 B8V
HR 3786 ψ CD-39 5580 82434 221234 W 4513 09 30 42.0 -40 28 00 3.60 F3IV+F0IV 0.5 0.7 D:4.1 F2IV, 4.6 F0V, 33.99y, a = 0.795". Combined mag., colors.,DYN:0.061".,VAR:Comp. B, 4.5 - 5.1v.
HR 3803 CP-56 2270 82668 237067 361 N Vel 09 31 13.3 -57 02 04 3.13 K5III VAR:L? 3.10 - 3.16V.
HR 3807 CD-40 5284 82694 221262 2759 W 09 32 19.3 -40 38 58 5.35 G8III 3.6 1.1
HR 3817 CD-48 4802 82984 221288 W 09 33 44.5 -49 00 18 5.12 B4IV 0.8 2.1 D:Secondary B8V, vsini 157k/s.,G:Sco-Cen assoc.; probable member of Sco-Cen cluster.,RV:Comp. A of double, RV var.; comp. B +20k/s.
HR 3819 CD-50 4270 83058 237107 2764 09 34 08.8 -51 15 19 5.01 B1.5IV
HR 3831 CD-48 4831 83368 221339 W IM Vel 09 36 25.3 -48 45 05 6.17 ApSrEuCr 2.4 3.1 RV:Detailed analysis by Kurtz and Marang (1988, MNRAS, 231, 1039) gives rotational frequency of 4.05829 microHz (2.85196d).,S:Also classified A7pSr.,VAR:Amp. 0.05V, 2.8519d. Also pulsations of 11.67 min.
HR 3836 CD-48 4836 83446 221344 2768 W 09 36 49.6 -49 21 19 4.35 A5IV-V 8.7 25.7
HR 3837 CP-52 2612 83465 237144 09 36 46.3 -52 56 39 6.19 K0III
HR 3840 CP-53 2646 83520 237149 W 09 37 12.3 -53 40 07 5.45 A2-3V 0.0 0.5 D:CPM.
HR 3842 CD-42 5462 83548 221355 2771 09 38 01.5 -43 11 28 5.50 G8II S:BaII star. Overabundance of praseodymium.
HR 3868 CP-54 2594 84228 237237 09 41 47.8 -55 12 51 6.00 B4V
HR 3872 CD-50 4420 84400 237260 W IP Vel 09 43 27.5 -51 13 42 6.15 B6V 4.7 2.1 VAR:E amp. 0.2b. Component A of visual double.
HR 3875 CP-53 2788 84461 237268 09 43 42.2 -53 53 30 5.56 A0IV G:Sco-Cen assoc.
HR 3886 CD-44 5846 84816 221484 Var? 09 46 30.4 -44 45 18 5.55 B2.5IV G:Sco-Cen assoc.
HR 3895 CP-55 2548 85250 237370 09 48 40.0 -56 24 43 6.06 K0III G:NGC 3033 #1.
HR 3898 CD-45 5470 85355 221523 W 09 49 57.1 -45 43 58 5.08 B7III 4.5 66.6 D:Secondary B9.
HR 3904 CD-46 5558 85483 221538 09 50 42.0 -46 56 04 5.73 K0IIICNIb
HR 3910 CD-45 5499 85563 221547 1256 09 51 19.8 -46 11 38 5.62 K2III
HR 3912 CD-45 5508 85622 221553 4658 09 51 40.8 -46 32 52 4.58 G5Ib SB:329.30d, K 14.1k/s, V0 +11.0k/s, asini 63.8.
HR 3920 CP-54 2816 85871 237448 4668 09 53 00.0 -55 22 24 6.48 B1IV VAR:6.3 - 6.36B.
HR 3924 CD-50 4622 85953 237464 Var? 09 53 50.2 -51 08 49 5.93 B2III VAR:BetaC, Amp. 0.03b, 0.1096d.
HR 3925 CD-44 5987 85980 221592 W 09 54 17.6 -45 17 02 5.71 B3V 2.4 5.3 D:Binary. Combined mag., colors.,G:Sco-Cen cluster.,RV:Component B, +5k/s.
HR 3927 CD-49 4801 86087 237483 09 54 51.3 -50 14 38 5.72 A0V SB:Equal components.
HR 3930 CD-40 5626 86211 221617 2795 09 56 05.4 -40 49 29 6.41 M1III
HR 3935 CD-50 4662 86352 237514 2797 09 56 21.9 -51 20 10 6.37 B2IV-V
HR 3940 φ CP-53 3075 86440 237522 375 W 09 56 51.8 -54 34 04 3.54 B5Ib 8.3 37.2 D:Companion K0III, optical.,G:Sco-Cen assoc.
HR 3941 CP-52 2980 86466 237526 IV Vel 09 57 10.9 -52 38 20 6.12 B3IV G:Sco-Cen assoc.; probable member of Sco-Cen cluster.,VAR:BetaC, amp. 0.013b, 0.1608d.
HR 3943 CD-47 5399 86523 221644 W 09 57 42.5 -48 24 52 6.05 B3V 4.6 14.1 D:CPM companion A0III; however, the companion is optical.
HR 3953 CP-56 2746 87030 237586 W 10 00 34.4 -56 56 48 6.52 K0III 6.5 7.6
HR 3955 CP-52 3087 87152 237612 Var? 10 01 40.5 -53 21 52 6.20 B2.5V G:Sco-Cen assoc.; doubtful member of the Sco-Cen cluster.
HR 3964 CD-46 5759 87363 221728 10 03 20.5 -46 38 10 6.12 A0V
HR 3976 CD-46 5806 87783 221773 W 10 06 11.3 -47 22 12 5.08 K1IV+G5V 1.7 0.7 D:5.3 K0IV, 6.9 G5V, 232y, a = 0.64". Combined mag., colors.
HR 3978 CD-51 4471 87816 237690 R Vel 10 06 07.1 -52 11 17 6.52 K1III VAR:Cst 6.49V.
HR 3990 CD-51 4507 88206 237736 10 08 56.3 -51 48 40 4.86 B3IV G:Sco-Cen assoc.
HR 4001 CD-41 5658 88399 221832 10 10 37.9 -41 42 54 5.98 K2-3III
HR 4010 CD-51 4560 88693 237784 10 12 23.0 -52 09 48 6.16 K2IIICNII
HR 4017 CD-50 4924 88824 237804 10 13 22.8 -51 14 00 5.28 A7V
HR 4020 CD-51 4578 88842 237807 W 4788 10 13 28.0 -51 45 22 5.78 A3IV-V 1.5 0.3
HR 4023 CD-41 5713 88955 221895 382 I 10 14 44.2 -42 07 19 3.85 A2V G:Sco-Cen assoc.
HR 4036 CD-42 6074 89062 221910 10 15 31.5 -43 06 45 5.60 K4III
HR 4038 CP-54 3356 89104 237834 Var? 10 15 16.6 -54 58 27 6.16 B2IV-V G:Sco-Cen assoc.; doubtful member of the Sco-Cen cluster.
HR 4045 CD-50 4990 89273 237858 GY Vel 10 16 40.2 -51 12 18 6.30 M4-5III VAR:Amp. 0.32V, 0.11R.
HR 4056 CD-41 5765 89461 221948 10 18 28.2 -41 40 06 5.96 B9V
HR 4061 CP-55 3220 89569 237902 10 18 37.6 -56 06 36 5.81 F6V
HR 4063 CP-54 3474 89682 237916 2830 GZ Vel 10 19 36.8 -55 01 46 4.57 K3II VAR:6.37 - 6.44P, 0.21R.
HR 4066 CD-47 5790 89736 221970 2831 10 20 16.7 -47 41 57 5.65 K5-M0III
HR 4074 CP-55 3286 89890 237959 W A 10 20 54.8 -56 02 35 4.50 B3IIIe v 3.7 7.1 D:AB binary?,VAR:Spectrum and H alpha vary.
HR 4080 CD-41 5809 89998 221998 1268 4837 10 22 19.6 -41 39 00 4.83 K1III
HR 4087 CD-41 5833 90170 222016 10 23 40.4 -41 57 12 6.27 G8IV G:Epsilon Ind group.
HR 4093 CD-41 5850 90393 222041 10 25 17.2 -42 28 05 6.18 G8III
HR 4099 CD-42 6222 90518 222047 10 26 09.5 -42 44 20 6.13 K1III
HR 4107 CP-54 3651 90677 238067 10 26 49.0 -54 52 39 5.58 K3II-III
HR 4111 CD-48 5655 90798 222081 4868 10 28 01.9 -49 24 20 6.10 K4III VAR:Amp. (U-B), 0.13.
HR 4134 CP-53 3909 91324 238146 W 10 31 21.8 -53 42 56 4.89 F6V 3.5 46.4 D:Companion K5, optical.,N:Called Y Argus in Velis by Lacaille 1763. Not the var. Y Vel.
HR 4135 CD-44 6583 91355 222126 W A 10 31 57.5 -45 04 00 5.74 B6II 0.4 13.7 D:Fixed with HR 4136. Mag. and color for combined light, 5.16V, -0.15(B-V), -0.62(U-B).
HR 4136 CD-44 6582 91356 222125 W B 10 31 56.6 -45 04 10 6.09 B8II 0.4 13.7 D:See HR 4135.
HR 4139 CD-43 6347 91437 222129 10 32 33.6 -44 37 08 5.91 G6-8III
HR 4143 CD-46 6205 91504 222136 1273 W 10 32 56.9 -47 00 12 5.02 K4III 4.0 40.2 D:CPM? Companion spectral class A.
HR 4154 CD-43 6395 91805 222170 W 10 35 10.5 -43 39 53 6.08 G8II-IIICNVp 8.4 14.7 S:Weak G-band.
HR 4167 CD-47 6042 92139 222199 I W 10 37 18.1 -48 13 33 3.84 F4IV+F3 0.9 0.3 D:4.2 F3IV+F0V, 5.1 A6V, 16.30y, a = 0.340".,DYN:0.022".,S:Also classified A3m F0-F2.,SB:Primary of visual double, 10.2104d, K 42.3k/s, V0 +21.2k/s, msin3i 0.333, asini 5.11.
HR 4175 CD-42 6390 92328 222222 2853 W 10 38 50.3 -42 45 13 6.11 Am+Am: 0.1 0.2
HR 4180 CP-54 3915 92449 238309 402 W 10 39 18.4 -55 36 12 4.28 G2-3Ib 2.2 51.8 D:Probably CPM. B is B8. C, 11.2v at 20" from B.,G:Red star Pleiades group.
HR 4216 μ CD-48 5913 93497 222321 I W 10 46 46.2 -49 25 12 2.69 G5III+G2V 3.7 1.7 D:2.7 G5III, 6.4 G2V, 116.24y, a = 1.437". Secondary also classified F8:V:.,G:Sirius group?
HR 4221 CP-56 3800 93563 238468 Var? 10 46 57.5 -56 45 26 5.23 B8-9IIIe v M:Old disk population runaway star.,S:Variable H alpha.,VAR:Suspected amp. 0.08V on time scale of 2 hrs.
HR 4263 CD-41 6220 94660 222422 KQ Vel 10 55 01.0 -42 15 04 6.11 A0pSiCr S:Magnetic field.,VAR:Appears to be variable over long time scale, especially toward uv (may be constant in V).
HR 4274 CD-50 5534 94985 238622 2874 IW Vel 10 57 07.9 -50 45 54 5.91 A4V VAR:Amp. 0.02B, 0.150d.
HR 4292 CD-43 6692 95347 222485 10 59 59.4 -43 48 26 5.81 B8-9V
HR 4293 CD-41 6276 95370 222487 415 11 00 09.3 -42 13 33 4.39 A3IV
HR 4296 CD-51 5220 95429 238674 W 11 00 08.6 -51 49 04 6.15 A3III-IV 7.1 10.3
HR 4311 CD-47 6466 96113 222538 2884 11 04 31.2 -47 40 45 5.67 A8III-IV
HR 4316 CD-48 6157 96224 222548 11 05 04.2 -49 23 33 6.13 B9.5V

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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