Catalogues

Catalogue

Constellation

Ursa Maior / 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 3182			BD+68 524	67447	14456	1215					08 12 48.8	+68 28 27	5.32	G7+II			N:Formerly called 55 Cam, in UMa.,S:Possible BaII star.
HR 3221			BD+60 1119	68457	14479				6680		08 15 50.5	+60 22 50	6.45	A7Vm	4.1	48.6	N:56 Cam, in UMa.
HR 3236			BD+72 409	68951	6504		I		6724		08 20 40.3	+72 24 26	5.98	M0III	3.7	42.9	D:B, 9.78V, +0.39(B-V), -0.02(U-B), F5IV.
HR 3245			BD+62 991	69148	14500					Var	08 19 17.3	+62 30 26	5.71	G8III			N:57 Cam, in UMa.,VAR:E? Amp. 0.062.
HR 3263			BD+61 1043	69976	14522						08 22 44.1	+60 37 52	6.41 R	K0III
HR 3303			BD+67 545	71088	14568	2662					08 29 46.2	+67 17 51	5.88	G8III
HR 3323	ο	1	BD+61 1054	71369	14573	317	I		6830	4093	08 30 15.9	+60 43 05	3.36	G5III	7.1	143.0	D:B is 15v at 7", CPM. C and D optical.,G:Probable Hyades group.,N:Muscida; a name also applied to Pi UMa, HR 3391, 3403.,VAR:3.3 - 3.8V, 358d. Also 0.05d, amp. 0.02V.
HR 3332			BD+69 472	71553	14582						08 32 53.4	+69 19 12	6.31	K0
HR 3354		2	BD+65 638	72037	14590						08 34 36.2	+65 08 42	5.47	A2m
HR 3391	π¹	3	BD+65 643	72905	14609						08 39 11.7	+65 01 15	5.64	G1.5Vb			G:Sirius group; UMa stream.,N:Muscida, with HR 3403.
HR 3400			BD+53 1268	73017	26935						08 38 22.2	+53 24 05	5.66	G8IV
HR 3401			BD+60 1148	73029	14612						08 39 10.2	+59 56 22	6.48	A2Vn
HR 3403	π²	4	BD+64 698	73108	14616	2677	I				08 40 12.8	+64 19 40	4.60	K1+IIIb			N:Muscida, with HR 3391.,S:Also classified K1IIIb CN-0.5.
HR 3405			BD+53 1269	73131	26940						08 39 00.0	+52 55 30	6.42 R	K0
HR 3408			BD+53 1272	73171	26946	323					08 39 17.6	+52 42 42	5.91	gK1			G:Probable Hyades group.
HR 3436			BD+47 1606	73971	42508						08 43 00.2	+46 54 04	6.22	G8III
HR 3470			BD+67 560	74604	14667						08 48 49.4	+66 42 29	6.20	B8V
HR 3505		5	BD+62 1027	75486	14691	2701					08 53 22.6	+61 57 44	5.73	F2III
HR 3506			BD+59 1198	75487	27026						08 53 05.9	+59 03 22	6.25 R	F5IV-V
HR 3531		6	BD+65 673	75958	14703						08 56 37.5	+64 36 14	5.58	G7IIIFe-0.5
HR 3569	ι	9	BD+48 1707	76644	42630	335	I		7114	4329	08 59 12.4	+48 02 30	3.14	A7IV	7.2	3.9	D:BC 10.8, 11.0, 39.69y, a = 0.68". BC is dM1. BCxA: 817.91y, a = 9.092". Separation rapidly decreasing. ADS 7114Aa,,D:11.02y, a = 90.354". This is the SB pair.,DYN:0.066".,G:Hyades group.,N:Talitha; Talita.,SB:ADS 7114A, 4028d, K 6.0k/s, V0 +6.8k/s, asini 310. Unresolved by speckle interferometry 1982.18.,VAR:ADS 7114A, S, 3.12 - 3.18V, 0.071d.
HR 3576	ρ	8	BD+68 551	76827	14742	338	I			4344	09 02 32.7	+67 37 47	4.76	M3III-IIIbCa1
HR 3592			BD+54 1272	77309	27105	340					09 04 00.4	+54 17 02	5.75	A2V
HR 3594	κ	12	BD+47 1633	77327	42661	341			7158	4357	09 03 37.5	+47 09 24	3.60	A1Vn	0.2	0.3	D:4.2 A0IV-V, 4.4 A0V, 70.1y, a = 0.27" or 64.29y, a = 0.26". Mag., colors for combined light.,DYN:0.009".
HR 3603			BD+49 1801	77601	42682						09 05 24.1	+48 31 49	5.95	F6II-III			S:Sr strong.
HR 3608			BD+59 1217	77692	27121	2716					09 06 43.1	+59 20 40	6.45	A2V
HR 3609	σ¹	11	BD+67 573	77800	14769		I				09 08 23.6	+66 52 24	5.14	K5III
HR 3616	σ²	13	BD+67 577	78154	14788				7203	4392	09 10 23.2	+67 08 05	4.80	F6IV	3.5	2.8	D:AB 4.85 F7IV-V, 8.16 K2V, 1067.1y, a = 6.20". C, probably optical.,DYN:0.044".,VAR:ADS 7203B, 7.5 - 10.0v?
HR 3619		15	BD+52 1365	78209	27136	2721					09 08 52.3	+51 36 17	4.48	F0IVm vs			S:Violet part of spectrum indicates luminosity III; G-band region, V. Also classified A1m.
HR 3624	τ	14	BD+64 723	78362	14796	2727			7211		09 10 55.1	+63 30 49	4.67	F3-4IIIm vs	6.2	57.2	D:B, optical.,S:Violet part of spectrum indicates luminosity III; G-band region, IV-V.,SB:ADS 7211A, 1062.4d, K 3.9k/s, V0 -8.7k/s, asini 50.0. Unresolved by speckle interferometry.
HR 3633			BD+72 444	78633	6784	2729					09 14 03.2	+71 39 21	6.55	G8III-IV
HR 3645			BD+73 452	78935	6792						09 15 52.6	+72 56 46	5.96	F0III
HR 3648		16	BD+62 1058	79028	14819	2730		W			09 14 20.6	+61 25 24	5.13	F9V			D:Noted by W. Herschel as double, sep. 49", is probably error: single star.,SB:16.2397d, K 35.3k/s, V0 -14.6k/s, asini 7.85.
HR 3660		17	BD+57 1211	79354	27185		I			4427	09 15 49.9	+56 44 29	5.27	K5III
HR 3662		18	BD+54 1285	79439	27191	2734				DD UMa	09 16 11.3	+54 01 19	4.83	A5V			G:Sirius group; UMa stream.,VAR:Delta Sct? Amp. 0.03V, 3 hrs., but sometimes cst. for 5 hrs.
HR 3676			BD+47 1658	79763	42790	2738					09 17 31.2	+46 49 02	5.97	A1V			G:Sirius group?,SB:15.986d, K 63.3k/s, V0 -13.1k/s, msin3i 1.49, asini 12.1.
HR 3697			BD+51 1495	80290	27215				7303		09 20 43.8	+51 15 58	6.13	F3V	4.0	142.1	D:AB, mag. diff 4.6v, binary.,DYN:0.034".
HR 3698			BD+57 1214	80390	27219	2743	I			CG UMa	09 21 43.3	+56 41 57	5.47	M4IIIa			VAR:Lb 5.87 - 5.95V.
HR 3722			BD+64 733	80953	14875		I				09 25 44.2	+63 56 27	6.28	K2III
HR 3725			BD+52 1389	81025	27246				7348		09 24 55.7	+51 34 26	6.31	G2III	2.2	1.4	D:CPM.,SB:ADS 7348A.
HR 3743			BD+46 1509	81688	42876	2751		W			09 28 40.0	+45 36 05	5.41	K0III-IV	2.5	77.3	N:41 Lyn in UMa.
HR 3747			BD+56 1388	81790	27271						09 29 47.6	+55 44 44	6.45 R	F3V s
HR 3757		23	BD+63 845	81937	14908	355	I		7402	4506	09 31 31.7	+63 03 43	3.67	F0IV	5.6	22.8	D:AB binary. C, 10.5v at 100", optical.,DYN:0.038".,G:Sirius group?,VAR:Delta Sct, amp. 0.07B, about 2 hrs.
HR 3768		22	BD+72 462	82189	6898					Var	09 34 53.6	+72 12 20	5.72	F7V			VAR:Amp. 0.025V, pulsating.
HR 3771		24	BD+70 565	82210	6897	357	I			DK UMa	09 34 28.9	+69 49 49	4.56	G4III-IV			VAR:Amp. 0.058V, 0.9202d, pulsating.
HR 3775	θ	25	BD+52 1401	82328	27289	358	I		7420	4519	09 32 51.4	+51 40 38	3.17	F6IV	10.7	4.1	D:CPM.,SB:371.0d, K 4.3k/s, V0 +13.0k/s, asini 21.24. Orbit questioned by Morbey and Griffin (1987, ApJ, 317, 343).,SB:Unresolved by speckle interferometry.
HR 3778			BD+50 1657	82380	42914						09 33 07.2	+49 26 19	6.76	A4V
HR 3797			BD+47 1683	82582	42924						09 34 19.6	+46 54 08	6.52	F0V
HR 3799		26	BD+52 1402	82621	27298						09 34 49.5	+52 03 05	4.50	A2V
HR 3824			BD+67 602	83126	14949	2769	I				09 39 27.9	+67 16 20	5.94	K5
HR 3838			BD+69 531	83489	14966	363					09 42 14.8	+69 14 15	5.69	gG9
HR 3839		27	BD+72 466	83506	6936	2772	I				09 42 57.2	+72 15 09	5.17	K0III
HR 3854			BD+49 1868	83869	42990	2774					09 42 43.1	+48 25 52	6.39	A1V
HR 3855			BD+55 1345	83886	27359	2775					09 43 07.0	+54 21 49	6.47	A5m
HR 3859			BD+65 731	83962	14976						09 44 36.7	+64 59 02	6.17 R	F3Vn
HR 3865		28	BD+64 752	84179	14980			W			09 45 55.4	+63 39 12	6.34	F2V	5.2	6.4	SB:Primary of visual double.
HR 3870			BD+57 1231	84335	27377		I			CS UMa	09 46 31.7	+57 07 41	5.20	M3IIIab			VAR:Amp. 0.16p.
HR 3881			BD+46 1551	84737	43046	1255					09 48 35.4	+46 01 16	5.09	G0.5Va
HR 3885			BD+66 637	84812	15000						09 50 23.7	+65 35 36	6.31	A9Vn
HR 3888	υ	29	BD+59 1268	84999	27401	368	I		7534	Ups UMa	09 50 59.4	+59 02 19	3.80	F2IV	8.6	11.3	D:CPM.,VAR:Delta Sct 3.77 - 3.86V, 0.133d, amp. and form of light curve vary.
HR 3894	φ	30	BD+54 1331	85235	27408				7545		09 52 06.4	+54 03 52	4.59	A3IV	0.2	0.3	D:5.30 A3IV, 5.38 A3IV, 105.5y, a = 0.360". Combined mag., colors.,DYN:0.008".,G:Possible Eggen group with HR 63, q.v.
HR 3911			BD+61 1151	85583	15023	2790		W			09 55 03.4	+61 06 58	6.27	K0	6.8	12.2
HR 3917		31	BD+50 1698	85795	27430	2793				SY UMa	09 55 43.0	+49 49 12	5.27	A3III			VAR:Cst? 5.23V.
HR 3918			BD+73 478	85841	7009	372					09 58 22.8	+72 52 46	5.83	gK3
HR 3922			BD+58 1224	85945	27438						09 57 13.6	+57 25 06	5.93	G5III			G:Wolf 630 group.
HR 3929			BD+46 1566	86166	43117	2798					09 57 56.9	+45 24 52	6.30	K0III
HR 3939			BD+57 1242	86378	27464	2802	I				09 59 51.7	+56 48 43	5.48	K5III
HR 3954			BD+54 1348	87141	27503	1259					10 04 36.3	+53 53 30	5.74	F5V
HR 3958			BD+53 1384	87243	27512						10 05 10.5	+52 22 15	6.14 R	A5IV
HR 4008			BD+60 1246	88651	15129	2821	I			U UMa	10 15 07.7	+59 59 08	6.25	M0III v			VAR:Cst? 6.25V.
HR 4021			BD+71 534	88849	7099				7705 A	4802	10 17 50.6	+71 03 38	6.66	A7m	0.7	16.6	D:AB binary. Both A and B Am stars. vsini both components =<25k/s. B is 7.36V, +0.30(B-V), +0.19(U-B).,DYN:0.007".,S:K/H/met lines indicate A6/F1/F2, respectively, for component A; A5/F0/F1 for component B.
HR 4026		32	BD+65 767	88983	15135	1262					10 18 02.0	+65 06 30	5.82	A8III
HR 4033	λ	33	BD+43 2005	89021	43268	383					10 17 05.8	+42 54 52	3.45	A2IV			G:Hyades group.,N:Tania Borealis. With HR 4069, Al Kafzah al Thaniyah.
HR 4044			BD+47 1761	89268	43281			W			10 18 59.0	+46 45 39	6.43	K1III	5.7	27.8
HR 4046			BD+49 1940	89319	43285	2827					10 19 26.8	+48 23 49	6.00	K0
HR 4047			BD+69 568	89343	15147	2828					10 21 03.4	+68 44 51	5.96	A7Vn
HR 4051			BD+54 1366	89389	27606						10 20 14.8	+53 46 45	6.45	F9V
HR 4052			BD+54 1367	89414	27609	2829					10 20 31.2	+54 13 01	6.00	gK3
HR 4067			BD+41 2076	89744	43309						10 22 10.5	+41 13 46	5.76	F7V
HR 4069	μ	34	BD+42 2115	89758	43310	386	I			4829	10 22 19.7	+41 29 58	3.05	M0III e			N:Tania Australis.,S:Ultraviolet FeII emission. H and K emission.,SB:230.089d, K 7.4k/s, V0 -20.4k/s, asini 23.4.,VAR:E?, 2.99 - 3.33V.
HR 4072			BD+66 664	89822	15163	387				4839	10 24 07.9	+65 33 59	4.97	A0pSiSr:Hg:			S:HgMn star; SrII 4077; Pt II.,SB:11.5791d, K 38.9k/s, V0 -2.6k/s, msin3i 0.754, asini 5.98.,VAR:Alpha CV?, 4.91 - 4.99V.
HR 4096			BD+42 2123	90470	43344						10 27 28.0	+41 36 03	6.02	A2V
HR 4098			BD+49 1961	90508	43351			W			10 28 03.8	+48 47 05	6.44	F9V	6.0	4.7	D:CPM.,G:Arcturus group.
HR 4103			BD+45 1832	90602	43356	2838					10 28 36.5	+45 12 44	6.35	K0
HR 4106		35	BD+66 671	90633	15196						10 29 54.3	+65 37 34	6.32	gK2
HR 4108			BD+64 789	90745	15200	2839					10 30 26.6	+64 15 27	6.12	A7III
HR 4112		36	BD+56 1459	90839	27670	394					10 30 37.6	+55 58 50	4.84	F8V	3.4	139.	D:Triple CPM and common RV system. B = BD+56d1458, 9.94pg; C = BD+57d1266, 8.99pg.
HR 4131			BD+54 1381	91311	27682						10 33 43.6	+53 29 51	6.45 R	A1V			S:Metal-deficient.
HR 4132			BD+41 2101	91312	43379	2844			7826		10 33 13.9	+40 25 32	4.75	A7IV	7.0	19.3	D:Visual companion optical.,SB:ADS 7826A, 292.56d, K 14.5k/s, V0 +9.0k/s, asini 55.6. Unresolved by speckle interferometry.
HR 4141		37	BD+57 1277	91480	27695	398					10 35 09.7	+57 04 58	5.16	F1V			G:"Dipper Stars"; Sirius group; UMa moving cluster.
HR 4165			BD+54 1387	92095	27724	2849	I				10 39 05.7	+53 40 06	5.52	K3III
HR 4176			BD+69 583	92354	15260		I				10 41 48.3	+68 26 36	5.75	gK3
HR 4178		38	BD+66 678	92424	15261	2855	I			4936	10 41 56.6	+65 42 59	5.12	K2III v
HR 4181			BD+69 586	92523	15269	403	I				10 43 04.1	+69 04 34	5.00	K3III-IIIb
HR 4187		39	BD+57 1286	92728	27748						10 43 43.3	+57 11 57	5.80	A0V s
HR 4191			BD+46 1657	92787	43444	1276		W			10 43 32.9	+46 12 14	5.18	F5III	2.8	286.9	D:AB CPM. B is GC 14751, dG0.,SB:Component B of visual double. RV amp. 45k/s.
HR 4195			BD+68 617	92839	15274		I			VY UMa	10 45 04.0	+67 24 41	6.00	C5II			S:Technetium found in spectrum.,VAR:Lb 5.89 - 6.5v.
HR 4202		41	BD+58 1281	93132	27760		I				10 46 22.5	+57 21 57	6.34	M1III			G:Eta Cep group.
HR 4215			BD+65 803	93427	15298						10 48 50.0	+65 07 56	6.39	A1V
HR 4235		43	BD+57 1294	93859	27791						10 51 11.1	+56 34 56	5.67	K2III
HR 4236		42	BD+60 1296	93875	27793	2865	I				10 51 23.7	+59 19 12	5.58	K2III
HR 4241			BD+53 1439	94083	27809						10 52 30.8	+52 33 55	6.65 R	gG8
HR 4242			BD+53 1440	94084	27810						10 52 31.9	+52 30 13	6.44	K2III
HR 4243			BD+70 634	94132	7229	2866		W			10 53 30.7	+69 51 14	5.93	G9IV	3.0	75.1
HR 4246		44	BD+55 1418	94247	27815	2869	I				10 53 34.5	+54 35 06	5.10	K3III			G:Hyades group.
HR 4248	ω	45	BD+43 2058	94334	43512	2870					10 53 58.7	+43 11 24	4.71	A1V s			SB:15.8307d, K 22.2k/s, V0 -18.7k/s, asini 4.59.
HR 4256			BD+34 2178	94497	62310						10 54 58.2	+34 02 05	5.72	gG7			N:47 LMi in UMa.
HR 4258		46	BD+34 2181	94600	62314		I				10 55 44.4	+33 30 25	5.03	K1III
HR 4264			BD+42 2162	94669	43535						10 56 14.5	+42 00 30	6.03	K2III			G:Wolf 630 group.
HR 4275			BD+52 1528	95057	27858	2876				5038	10 59 17.9	+51 52 56	6.17	K0			VAR:6.0 - 7.4p. Faint only Feb. 6, 1943.
HR 4277		47	BD+41 2147	95128	43557	1282					10 59 28.0	+40 25 49	5.05	G1-VFe-0.5
HR 4278			BD+36 2139	95129	62345		I				10 59 32.8	+36 05 35	6.00	M2III
HR 4280			BD+46 1680	95212	43562	2878	I				11 00 14.7	+45 31 34	5.47	K5III
HR 4283			BD+52 1529	95233	27868						11 00 25.6	+51 30 07	6.43	G9III
HR 4285			BD+43 2068	95241	43564			W			11 00 20.6	+42 54 41	6.02	F9V	5.6	37.1
HR 4286			BD+64 824	95256	15360						11 01 05.8	+63 25 16	6.39	A2Vm
HR 4288		49	BD+39 2400	95310	62354						11 00 50.4	+39 12 44	5.08	F0V s			S:Also classified F0m, F0IV, Am.
HR 4295	β	48	BD+57 1302	95418	27876	416	I			5053	11 01 50.5	+56 22 57	2.37	A1V			G:"Dipper Stars;" UMa cluster; Sirius group; UMa stream.,N:MERAK; Mirak.
HR 4301	α	50	BD+62 1161	95689	15384	417	I		8035	5070	11 03 43.7	+61 45 03	1.79	K0IIIa e	3.0	0.5	D:1.87 K0III, 4.81 F0V, 44.4y, a = 0.603". Also classified K0II-III + A8V:. Combined mag., colors. Also CPM at 280",D:with HD 95638 = GC 15179, 7.12V F8; SB, 6.04d.,DYN:0.039".,N:DUBHE; Dubb; Ak.,S:Balloon-borne spectrometer revealed pronounced emission of MgII.,SB:44.0y, K 2.0k/s, V0 -8.7k/s, asini 414. Unresolved by speckle interferometry.,VAR:ADS 8035A; B also var. suspect NSV 5071, too close to primary to be certain of variability.
HR 4309		51	BD+39 2414	95934	62387	2882			8046		11 04 31.2	+38 14 29	6.00	A3III-IV	7.1	8.4	D:AB, CPM.
HR 4330			BD+68 632	96707	15414					Var?	11 09 39.9	+67 12 37	6.06	F0pSr v			S:Probable magnetic star.,VAR:Large spectrum var., 0.8183d (not confirmed). Amp. 0.02V. HR 4340 used as comparison star.
HR 4333			BD+37 2162	96813	62427	2892	I			CO UMa	11 09 19.1	+36 18 34	5.74	M3.5IIIab			G:Zeta Her group.,VAR:Lb? 5.79 - 5.95V.
HR 4335	ψ	52	BD+45 1897	96833	43629	420	I				11 09 39.8	+44 29 55	3.01	K1III
HR 4336			BD+43 2083	96834	43627		I			5107	11 09 38.5	+43 12 27	5.89	M2III			G:Epsilon Ind group.
HR 4340			BD+69 602	97138	15431					5119	11 12 11.0	+68 16 19	6.40	A3V
HR 4344			BD+55 1446	97302	27952						11 12 44.5	+54 53 39	6.63	A4V
HR 4345			BD+36 2162	97334	62451			W			11 12 32.2	+35 48 49	6.41	G0V	1.6	138.7
HR 4351			BD+41 2170	97501	43649				8093		11 13 40.2	+41 05 19	6.33	K2III	4.8	3.1	D:Fixed sep.
HR 4363			BD+53 1480	97855	27970				8108 A		11 16 04.0	+52 46 23	6.50	F6V+F9V	1.7	12.7	D:CPM.,S:Also classified F2, F6V.
HR 4367			BD+50 1807	97989	43675	424					11 16 41.9	+49 28 35	5.88	gK0
HR 4374	ξ	53	BD+32 2132	98230	62484		I		8119 B	5165	11 18 10.9	+31 31 45	4.87 H	G0V	0.5	3.1	D:Binary with HR 4375, q.v.,DYN:0.120".,S:Xi UMa B has low lithium abundance while its companion has high.,SB:3.9805d, K 5.0k/s, V0 -15.9k/s, asini 0.274. Unresolved by speckle interferometry 1982.17.,VAR:Blend of 4374-5. Amp. 0.03V.
HR 4375	ξ	53	BD+32 2132	98231	62484		I		8119 A	5165	11 18 11.0	+31 31 45	4.41 H	G0V	0.5	3.1	D:AB 4.32 G0V, 4.79 G0V, 59.840y, a = 2.530". Combined colors. Mag. for blend 3.79V. AB, first visual double for which an,D:orbit determined, in 1828 by Savary. Third component astrometric with A, 1.832y, a = 0.055".,DYN:0.120".,N:Alula Australis.,SB:ADS 8119A, 669.18d, K 8.0k/s, V0 -15.0k/s, asini 62.4. SB same per. as orbital astrometric binary AP. Resolved,SB:by speckle interferometry.,VAR:See HR 4374.
HR 4377	ν	54	BD+33 2098	98262	62486	425	I		8123		11 18 28.7	+33 05 39	3.48	K3-IIIBa0.3	6.0	7.2	D:CPM.,DYN:0.005".,N:Alula Borealis.
HR 4380		55	BD+38 2225	98353	62491	1293					11 19 07.9	+38 11 08	4.78	A1Vp:			S:Lambda Boo star, Mg 4481 wk:,SB:2.55385d, K 80.4k/s, V0 -4.6k/s, asini 2.54. Insufficient broad-line velocities determined to permit two-component,SB:solution; however, velocities consistent with mass ratio of about 0.9 (Lloyd 1981).
HR 4383			BD+67 692	98499	15478	2905					11 20 53.8	+67 06 02	6.21	G8
HR 4388			BD+57 1316	98673	27999	2907					11 21 49.3	+57 04 30	6.43	A7Vn
HR 4391			BD+65 828	98772	15486	429					11 22 51.3	+64 19 50	6.02	A1Vnp			S:Lambda Boo star, Mg 4481 wk.
HR 4392		56	BD+44 2083	98839	43719	2908	I				11 22 49.6	+43 28 58	4.99	G7.5IIIa:Ba0.3
HR 4407			BD+56 1518	99283	28017						11 25 57.1	+55 51 02	5.75	K0III
HR 4412			BD+34 2222	99373	62551						11 26 25.5	+33 27 02	6.32	F7V
HR 4421			BD+62 1183	99747	15520	2915					11 29 04.6	+61 46 42	5.83	F5Va vw
HR 4422		57	BD+40 2433	99787	62572				8175		11 29 04.2	+39 20 13	5.31	A2V	2.5	346.3	D:ADS 8175AB, 8.2 dG5, 4500y.,DYN:0.021".
HR 4424			BD+57 1324	99859	28035						11 29 43.5	+56 44 15	6.28	A4m			S:Also classified A5V.
HR 4427			BD+55 1468	99913	28038						11 30 12.9	+54 21 42	6.41 R	K0III
HR 4430			BD+47 1880	99967	43784					EE UMa	11 30 25.0	+46 39 27	6.35	K2IIICN-1			SB:74.861d, K 28.8k/s, V0 +27.9k/s, asini 29.6. Unresolved by speckle interferometry.,VAR:Ell:, amp. 0.13V, 39d x 2?
HR 4431		58	BD+43 2122	99984	43787	432					11 30 31.1	+43 10 24	5.94	F4V			S:Also classified F7III.
HR 4435			BD+48 1952	100030	43790						11 30 52.9	+47 55 45	6.42	G9IV
HR 4436			BD+49 2062	100055	43793						11 31 10.2	+48 47 21	6.56	G9III
HR 4439			BD+61 1246	100203	15542				8197		11 32 20.8	+61 04 57	5.48	F8V	1.4	0.5	D:5.75 F6V, 7.07 G3V, 72.87y, a = 0.813". Combined mag., colors.,DYN:0.034".
HR 4452			BD+37 2195	100470	62604	2923					11 33 56.3	+36 48 56	6.40	K0III			G:Sigma Pup group.
HR 4457			BD+55 1473	100615	28064	2925					11 35 04.9	+54 47 07	5.63	K0III
HR 4474			BD+51 1679	101013	28081	2929					11 37 53.0	+50 37 06	6.14	G9III:Ba2.5
HR 4477		59	BD+44 2110	101107	43837						11 38 20.6	+43 37 32	5.59	F2II-III
HR 4480		60	BD+47 1894	101133	43839	2931					11 38 33.5	+46 50 03	6.10	F5III s
HR 4481			BD+65 843	101150	15580				8249		11 38 49.2	+64 20 49	6.46 R	A5IV	1.3	1.8
HR 4482			BD+34 2242	101151	62635						11 38 32.2	+33 37 32	6.27	K2III
HR 4486			BD+45 1947	101177	43841				8250 A		11 38 44.9	+45 06 31	6.44	G0V	1.9	9.4	D:AB binary.,DYN:0.044".,RV:ADS 8250A, -18k/s; B -14k/s; C -40k/s.,SB:ADS 8250B, dK5, 23.5415d, K 25.8k/s, V0 -13.8k/s, asini 7.82.
HR 4493			BD+58 1331	101391	28093						11 40 27.4	+57 58 14	6.37	B9pHgMn:
HR 4496		61	BD+35 2270	101501	62655	1300		W		5291	11 41 03.0	+34 12 06	5.33	G8V	4.9	159.3
HR 4500			BD+55 1481	101604	28101		I				11 41 43.6	+55 10 21	6.27	K5
HR 4501		62	BD+32 2179	101606	62658	2938		W			11 41 34.3	+31 44 46	5.73	F4V	4.3	84.3	D:Resolved by speckle interferometry 1986.44, sep. 0.03".
HR 4518	χ	63	BD+48 1966	102224	43886	441	I			5319	11 46 03.0	+47 46 46	3.71	K0.5IIIb			N:Discordances as to whether Xi or Iota and Kappa UMa (HR 3569, 3594) should be El Koprah, Alkaphrah.,VAR:Amp. 0.04V?
HR 4521			BD+56 1544	102328	28142	2941	I				11 46 55.6	+55 37 42	5.27	K2.5IIIbCN1Ca1
HR 4536			BD+35 2284	102713	62718						11 49 41.7	+34 55 54	5.70	F5IV			SB:32.864d, K 37.3k/s, V0 -8.3k/s, asini 16.8.
HR 4545			BD+34 2264	102942	62731			W			11 51 09.4	+33 22 30	6.27	Am	2.5	46.6
HR 4550			BD+38 2285	103095	62738	1307				CF UMa	11 52 58.8	+37 43 07	6.45	G8Vp	5.5	1.7	D:The reality of the companion, CF UMa, announced by P. van de Kamp (see Low Luminosity Stars, ed. S. S. Kumar, p. 199,,D:1968) has been questioned (PASP, 96, 557, 1984). Unresolved by speckle interferometry 1980.47.,N:Groombridge 1830.,VAR:Companion of Groombridge 1830, UV? 8.5-12v.
HR 4554	γ	64	BD+54 1475	103287	28179	447	I			5379	11 53 49.8	+53 41 41	2.44	A0Ve			C:Color excess E(B-V) = 0.00.,G:"Dipper Stars;" Sirius group; UMa moving cluster.,N:PHAD; Phecda; Phekda; Phegda; Phekha; Phacd.,S:Variable emission of K line and possible variation in H alpha.
HR 4560		65	BD+47 1913	103483	43945				8347 A	DN UMa	11 55 05.7	+46 28 37	6.54	A3Vn	0.4	63.0	D:Binary with HR 4561 = ADS 8347D. AB binary 7.2, 9.0 sep. 0.3". ABxC, 8.4 at 4" also binary.,VAR:Amp. 0.09B, 0.87d? Uncertain which of components A, B, C of ADS 8347 is the var.
HR 4561		65	BD+47 1914	103498	43946				8347 D		11 55 11.2	+46 28 11	7.03	A1pCrEuSr:	0.4	63.0	D:See HR 4560.,RV:78 Vir type.
HR 4562			BD+37 2230	103500	62754		I				11 55 14.1	+36 45 23	6.49	M3III
HR 4566		66	BD+57 1343	103605	28191	2953					11 55 58.4	+56 35 55	5.84	K1III
HR 4569			BD+62 1204	103736	15666						11 56 53.2	+61 32 57	6.22	G8III
HR 4572			BD+41 2253	103799	43963	2954					11 57 14.6	+40 20 37	6.62	F6V
HR 4574			BD+33 2174	103928	62774	1310			8368		11 58 07.2	+32 16 26	6.42	A9V	5.0	122.5	D:AB, CPM. B, 12.5v at 7". D, 12v at 140".
HR 4575			BD+62 1206	103953	15673						11 58 20.6	+61 27 53	6.76	K0III
HR 4581			BD+33 2176	104075	62784				8374		11 59 17.6	+33 10 03	5.96	K1III	6.0	4.5	D:Fixed sep.
HR 4584			BD+34 2279	104179	62786						11 59 57.2	+34 02 06	6.50	A9III
HR 4593			BD+36 2230	104438	62802	2963					12 01 39.5	+36 02 31	5.59	K0III
HR 4594		67	BD+43 2179	104513	44002	2965		W		DP UMa	12 02 06.8	+43 02 44	5.21	F0Vam	1.7	310.5	S:Also classified A4m, A7m.,VAR:Delta Sct amp. 0.02V, 0.04d - 0.08d, possible beat phenomena.
HR 4610			BD+63 999	105043	15710				8417	5452	12 05 39.7	+62 55 59	6.13	K2III	5.4	2.3	D:CPM.,VAR:ADS 8417B, 10.4 - 11.4?v.
HR 4641		68	BD+57 1359	106002	28291		I				12 11 44.9	+57 03 16	6.43 R	gK5
HR 4654			BD+54 1504	106478	28309	1314					12 14 43.4	+53 26 05	6.16	gK0			N:1 CVn in UMa.
HR 4660	δ	69	BD+57 1363	106591	28315	456		W		5513	12 15 25.6	+57 01 57	3.31	A3V	6.6	189.6	G:"Dipper Stars"; Ursa cluster; Sirius group; UMa stream.,N:MEGREZ; Kaffa in Becvar.
HR 4672			BD+54 1510	106884	28327		I				12 17 29.5	+53 11 28	5.81	K6III
HR 4701		70	BD+58 1371	107465	28346		I				12 20 50.8	+57 51 50	5.55	K5III
HR 4726		71	BD+57 1373	108135	28375		I				12 25 03.2	+56 46 39	5.81	M3IIIb
HR 4745		73	BD+56 1598	108502	28394	3000	I				12 27 35.1	+55 42 46	5.70	M2IIIb
HR 4760		74	BD+59 1444	108844	28405	467					12 29 57.3	+58 24 21	5.35	A5Del Del
HR 4762		75	BD+59 1446	108861	28408						12 30 04.3	+58 46 03	6.08	G8III-IV
HR 4767			BD+53 1554	108954	28413						12 30 50.1	+53 04 36	6.21	F8-G0V
HR 4800			BD+60 1406	109729	28444		I			T UMa	12 36 23.3	+59 29 13	5.50 H	M4IIIe			VAR:M 6.6 - 13.4v, 256.54d.
HR 4833		76	BD+63 1026	110462	15871	478					12 41 33.9	+62 42 47	6.07	A2III
HR 4840			BD+61 1312	110678	15877					Var	12 43 04.2	+61 09 20	6.38	K0			VAR:Amp. 0.07V.
HR 4859			BD+63 1034	111270	15901						12 47 18.9	+62 46 51	5.89 R	A9V
HR 4867			BD+61 1320	111456	15907						12 48 39.4	+60 19 12	5.85	F5V			G:UMa cluster; Sirius group.
HR 4905	ε	77	BD+56 1627	112185	28553	483	I			Eps UMa	12 54 01.7	+55 57 35	1.77	A0pCr			G:"Dipper Stars;" Sirius group; UMa stream; UMa moving cluster.,N:ALIOTH; Aliath.,R:4 solar radii.,S:Also classified A0pCrMn.,SB:0.95d and 4.15y. SB unresolved by speckle interferometry 1980.47. Binary nature questioned. Rotational period 5.09d.,VAR:Alpha CV 1.76 - 1.79V, 5.0887d. Spectrum variable. Photometric var. due to UV absorption from overabundant metals.
HR 4917			BD+54 1556	112486	28572				8710		12 56 17.6	+54 05 58	5.82	A5m	1.8	3.5	D:AB binary? C, 10.4v at 124" optical?,S:Also classified A2V.,SB:5.1274d, K 69.9k/s, V0 +7.3k/s, msin3i 0.609, asini 4.92. Possibly eclipsing? vsini both components 20k/s.
HR 4931		78	BD+57 1408	113139	28601				8739	6058	13 00 43.8	+56 21 59	4.93	F2V	2.5	1.3	D:5.05 F2V, 7.43 G6V, 109.97y, a = 1.270" or 106.7y, a = 1.281". Combined mag., colors.,DYN:0.039".,G:"Dipper Stars;" Sirius group; UMa stream; UMa moving cluster.,VAR:ADS 8739B, 7.5 - 10.5v.
HR 4936			BD+60 1439	113436	28613	3041					13 02 40.4	+59 42 58	6.53	A3Vn
HR 4953			BD+62 1275	113994	15985						13 06 22.7	+62 02 31	6.14	G7III
HR 4974			BD+63 1056	114504	15999	3050		W			13 09 50.2	+62 13 45	6.54	A1V	3.2	107.8
HR 5054	ζ	79	BD+55 1598	116656	28737	497	I		8891 A	6224	13 23 55.5	+54 55 31	2.27	A1VpSrSi	1.7	0.0	D:Aa = AP 3.0 A2V, 3.0 A2V, sep. 0.0115", 0.056y, a = 0.012". Combined mag., colors AP. Binary with HR 5055. Alcor,,D:HR 5062, at 709", CPM.,DYN:0.046".,G:"Dipper Stars;" Sirius group; UMa moving cluster.,N:MIZAR; Mizat; Mirza.,S:Combined spectrum for Aa also classified A1VpSrSi.,SB:ADS 8891Aa, 20.5386d, K 68.8k/s, V0 -5.6k/s, msin3i 1.60, asini 16.4. i 60d. vsini both components 32k/s. The,SB:first SB to have been discovered, by Pickering in 1889. First resolved by 20-foot interferometer at Mt. Wilson by Pease,SB:in 1925, sep. 0.01".
HR 5055	ζ	79	BD+55 1598	116657	28738		I		8891 B	6225	13 23 56.4	+54 55 18	3.95	A1m	1.7	0.0	D:Binary with HR 5054, q.v. Sep. 14". ADS 8891B also astrometric binary, 57y, a = 0.13".,DYN:0.046".,G:UMa stream; UMa cluster; Sirius group.,S:K/H/met lines indicate A1/A2/A7, respectively. Also classified A2/A7/A9 and A7Vm.,SB:ADS 8891B, 175.55d, K 6.3k/s, V0 -9.3k/s, asini 13.5.
HR 5062		80	BD+55 1603	116842	28751					6238	13 25 13.5	+54 59 17	4.01	A5V			D:CPM with HR 5054-5.,G:"Dipper Stars;" Sirius group; UMa stream; UMa moving cluster.,N:ALCOR; Saidak.,VAR:Delta Sct.
HR 5070			BD+64 949	117043	16071						13 25 59.9	+63 15 40	6.50	G6V			VAR:First known potassium flare star.
HR 5076			BD+53 1622	117242	28763						13 27 59.5	+52 44 45	6.34	F0
HR 5085			BD+60 1461	117376	16080	500		W			13 28 27.1	+59 56 45	5.40	A1Vn	3.3	182.3	G:Hyades group.
HR 5109		81	BD+56 1667	118214	28803					6319	13 34 07.3	+55 20 55	5.60	A0V
HR 5126			BD+50 2014	118536	44682						13 36 39.8	+49 29 12	6.49 R	K1III
HR 5133			BD+51 1856	118741	28819		I		8979		13 37 43.0	+50 42 53	6.48	M2II-III+K3III:	1.3	1.8	D:Binary. Companion K3III.
HR 5142		82	BD+53 1640	119024	28832						13 39 30.4	+52 55 17	5.46	A3Vn
HR 5148			BD+51 1859	119124	28836				8992		13 40 23.2	+50 31 10	6.32	F7-9V	4.3	17.6	D:CPM.
HR 5153			BD+57 1456	119213	28838					CQ UMa	13 40 21.3	+57 12 27	6.29	A2VpSrCrEu v			VAR:Alpha CV 6.24 - 6.26V, 2.449909+/-0.000011d, asymmetric light curve. Spectrum var.
HR 5154		83	BD+55 1625	119228	28843	3087	I			6389	13 40 44.3	+54 40 54	4.66	M2IIIabBa0.5
HR 5169			BD+52 1733	119765	28866						13 43 54.7	+52 03 52	6.02	A1V
HR 5177			BD+56 1683	119992	28878						13 45 13.2	+55 52 46	6.50	F7IV-V
HR 5187		84	BD+55 1634	120198	28885					CR UMa	13 46 35.7	+54 25 58	5.70	B9pEuCr v			VAR:Alpha CV 5.64 - 5.67V, 1.37996d, amp. 0.03U. Spectrum variable.
HR 5191	η	85	BD+50 2027	120315	44752	509	I			6450	13 47 32.4	+49 18 48	1.86	B3V			C:Color excess E(B-V) = +0.02.,G:Cas-Tau OB1; member of Pleiades group.,N:ALKAID; Benetnash; Benetnasch; Elkeid.,S:Lyman alpha observed from COPERNICUS.
HR 5213			BD+62 1318	120787	16186	3101					13 49 45.5	+61 29 21	5.96	G3V
HR 5216			BD+59 1533	120874	28901						13 50 27.7	+58 32 22	6.46	A3V
HR 5238		86	BD+54 1630	121409	28928						13 53 51.0	+53 43 43	5.70	A0V
HR 5256			BD+62 1325	122064	16230						13 57 32.1	+61 29 34	6.37 R	K3V
HR 5280			BD+51 1889	122866	28989						14 02 59.7	+50 58 19	6.15	A2V
HR 5302			BD+60 1516	123977	29019	3126					14 08 46.0	+59 20 16	6.46	K0III

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

Ursa Maior / Yale Bright Star Catalog (HR)

Legend

References