Catalogues

Catalogue

Constellation

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)

Catalogues

Vela / Yale Bright Star Catalog (HR)

Legend

References