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Katalog

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Auriga / 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 1501			BD+32 827	29867	57393						04 43 48.3	+32 51 55	6.45 R	A8V
HR 1528			BD+32 840	30453	57444			S			04 49 19.0	+32 35 18	5.86	A8m			SB:7.0507d, K 57.8k/s, V0 +20.3k/s, asini 5.60.
HR 1529			BD+31 816	30454	57441	2359	I				04 49 12.8	+31 26 14	5.58	K2III
HR 1535			BD+48 1162	30557	39799	2361					04 51 09.3	+48 44 27	5.66	G9III
HR 1550			BD+42 1081	30823	39826						04 52 47.8	+42 35 12	5.71	A3III
HR 1551		2	BD+36 952	30834	57475		I				04 52 38.0	+36 42 11	4.78	K2.5IIIbBa0.4			G:Sirius group; UMa stream.
HR 1558			BD+43 1116	31069	39851						04 54 51.3	+44 03 39	6.08	A0V
HR 1573			BD+35 930	31327	57511						04 56 19.9	+36 10 08	6.07	B2Ib			G:Aur OB1.
HR 1577	ι	3	BD+32 855	31398	57522	181	I			1778	04 56 59.6	+33 09 58	2.69	K3II			N:Hassaleh in Becvar.,VAR:4.0 - 4.15p.
HR 1592	ω	4	BD+37 1005	31647	57548				3572		04 59 15.4	+37 53 25	4.94	A1V	2.8	5.1	D:Binary.,DYN:0.021".,G:Pleiades group.
HR 1599		5	BD+39 1133	31761	57559				3589		05 00 18.3	+39 23 41	5.95	F5V	3.4	3.7	DYN:0.037".
HR 1602		6	BD+39 1134	31780	57560		I				05 00 23.2	+39 39 18	6.58 R	K4I
HR 1605	ε	7	BD+43 1166	31964	39955	183	I		3605	Eps Aur	05 01 58.1	+43 49 24	2.99	F0Iae+B v	6.2	207.6	D:ADS 3605A. A* 2.98 var. A8Iap. Five visual and one astrometric components. AB visual binary, B, 14v at 29"; C,,D:11.26V, +1.83(B-V), +1.31(U-B), at 43"; D, 12.0v at 46".,N:Al Anz; Almaaz.,S:Shell star. Also classified A8Ia-F2epIa + B.,SB:ADS 3605A, 9890d, K 15.0k/s, V0 -1.4k/s, msin3i 16.8, asini 2000. Unresolved by speckle interferometry.,VAR:ADS 3605A, EA 2.94 - 3.83V, 9892d. Spectrum var. even outside eclipse. RV and light fluctuations about 110d.
HR 1612	ζ	8	BD+40 1142	32068	39966	1137	I			Zet Aur	05 02 28.7	+41 04 33	3.75	K4II+B8V			N:Haedi; Haedus; Hoedus I. With HR 1641, one of the "kids"; Sadatoni; Saclateni.,S:Also classified K5II + B5V.,SB:972.162d, K 24.6k/s, V0 +12.9k/s, msin3i 7.54, asini 300. Unresolved by speckle interferometry . SKYLAB,SB:indicates cool star with hot companion.,VAR:EA 3.70 - 3.97V, 972.164d, i 90d. Variable duration of min. Amp. depends on wavelength, 0.55B, 1.97U. K component,VAR:amp. 0.05V.
HR 1615			BD+41 1044	32188	39979					1810	05 03 18.6	+41 26 30	6.14	A2IIIShell?			S:H alpha, beta and gamma have absorption cores. TiII and FeII stronger than normal; MgII, SiII strong. Shell doubtful.
HR 1626			BD+30 772	32406	57610						05 04 14.5	+30 29 41	6.14	K0II-III
HR 1627			BD+32 879	32428	57614						05 04 36.9	+32 19 13	6.62	A4m			S:Also classified A8.5Vm:
HR 1637		9	BD+51 1024	32537	25019				3675		05 06 40.6	+51 35 52	5.00	F0V	4.4	90.1	D:A,B,C, CPM; D, optical; E, 12.3v at 132" from A.,SB:ADS 3675A, 391.7d, K 5.8k/s, V0 -7.4k/s, asini 29.0.
HR 1639			BD+35 973	32608	57629	2379					05 06 00.9	+35 56 11	6.52	A5V
HR 1641	η	10	BD+41 1058	32630	40026	185				1822	05 06 30.9	+41 14 04	3.17	B3V			G:Cas-Tau OB1; member of Pleiades group.,N:Hoedus II. One of the kids, with HR 1612.,RV:Doubtful var., 24d period not confirmed.,VAR:Beta C?
HR 1644			BD+42 1170	32655	40029						05 06 49.6	+43 10 29	6.20	F2IIp:
HR 1668			BD+46 970	33167	40077						05 10 42.9	+46 57 44	5.68	F5V			G:Hyades moving group.
HR 1669			BD+37 1067	33203	57704		I		3734		05 10 18.9	+37 18 07	6.02	K3:+B2II:	0.1	1.5	D:AB, CPM.
HR 1689	μ	11	BD+38 1063	33641	57755	192					05 13 25.7	+38 29 04	4.86	A4Vm
HR 1692			BD+53 872	33654	25087	2393					05 14 44.3	+53 12 50	6.20	A0V
HR 1706		14	BD+32 922	33959	57799				3824 A	KW Aur	05 15 24.4	+32 41 16	5.02	A9IVDel Del	2.9	14.3	D:AC binary. B, 11v F4V at 13" optical.,G:Possible new Eggen group with HR 63, q.v.,SB:ADS 3824A, 3.788506d, K 23.0k/s, V0 -9.8k/s, asini 1.20.,VAR:Delta Sct 4.94 - 5.10V, 0.088088d. Form of light curve varies. Also nonradial pulsations of 0.096533 and 0.088243d.
HR 1707			BD+53 882	34019	25112		I		3845	R Aur	05 17 17.8	+53 35 10	6.50	M7IIIe	2.1	46.4	D:Binary. Component B, 9.50V, +0.47(B-V), +0.09(U-B), F4IV.,S:Probable SiO maser emission.,VAR:ADS 3845A, M 6.7 - 13.7v, 457.64d, period changes; 10.18 - 13.12V, -0.06 to -0.43(U-B). Cycle of 64.5d also possible.
HR 1708	α	13	BD+45 1077	34029	40186	193	I		3841	1897	05 16 41.4	+45 59 53	0.08	G5IIIe+G0III v	0.5	0.0	D:AP 0.6 G5III, 1.1 G0III, sep. 0.04", 0.285y, a = 0.054", masses 2.67 and 2.55 solar. Combined mag., colors. Capella is,D:first star for which an orbit was determined from interferometer measures, by Anderson at Mt. Wilson in 1920. Speckle,D:sep. 0.040" 1981.24 and 1981.68; 0.055" 1982.16. CPM with component H, a close binary, 10.0 dM1, 13.7 dM5 sep. 2" at,D:723" from A, probably physical with A. Other components all faint and distant from A.,DYN:0.058".,G:Hyades group.,N:CAPELLA; Alhajoth.,R:Diam. component A = 0.0052", component B = 0.0040".,S:Chromospheric He 10830 double. Balloon-borne spectrometer revealed pronounced emission of MgII. Soft X-ray emission.,S:Lithium content of the F-type component is 15 times that of the G component. Also classified G6III+F9III.,SB:104.0204d, K 26.1k/s, V0 +29.5k/s, asini 37.3.,VAR:Amp. 0.03V. Variable helium and X-ray emission.
HR 1712			BD+34 980	34078	57816				3843	AE Aur	05 16 18.2	+34 18 43	5.96	O9.5V e	3.3	8.4	D:Component B doubtful, possibly the nebula. C 10.7V at 30".,G:Runaway star from Ori OB1 association. Moving at 128k/s in opposite direction from Mu Col = HR 1996. See HR 938.,G:Exciting star of HII region S229; associated with nebula IC 405. S229 superimposed on S230. In reflection nebula. The,G:best example of nebulosity in which the gas and dust are differently distributed.,S:Central Balmer emission in blue-violet only.,VAR:ADS 3843A, Ina 5.78 - 6.08V. Possibly a SN 2.5 million yrs. ago.
HR 1722			BD+42 1239	34269	40214		I			PU Aur	05 18 15.9	+42 47 32	5.48	M4III			VAR:Lb?, amp. 0.10V.
HR 1725			BD+40 1240	34332	40224						05 18 40.4	+40 27 54	6.18	K0
HR 1726		16	BD+33 1000	34334	57853		I		3872	1909	05 18 10.7	+33 22 18	4.54	K2.5IIIbFe-1	5.8	4.2	D:CPM.,S:Also classified K2.5IIIb CN-0.5.,SB:ADS 3872A, 434.8d, K 14.8k/s, V0 -27.5k/s, asini 88.0.,VAR:ADS 3872A, E?
HR 1728		17	BD+33 1002	34364	57858					AR Aur	05 18 18.9	+33 46 02	6.14	B9.5V			D:Possible CPM with HR 1732.,G:Aur OB1. Concentration of hydrogen emission in direction of this association.,S:Also classified ApHgMn + B9V.,SB:4.1346d, K 107.2k/s, V0 +25.1k/s, msin3i 2.48, asini 6.09; vsini of secondary 62k/s.,VAR:EA 6.15 - 6.82V, 6.05 - 6.72B, A0 + A0, 4.134695d, changing period.
HR 1729	λ	15	BD+39 1248	34411	40233	1145			3886		05 19 08.5	+40 05 57	4.71	G1.5IV-VFe-1	4.9	146.6	D:B, 13.4v at 29". C, 12.1v at 42" and D, optical.,G:Epsilon Ind group.
HR 1732			BD+33 1008	34452	57884					IQ Aur	05 19 00.0	+33 44 54	5.41	A0pSi v			D:Possible CPM with HR 1728.,S:Magnetic star showing chlorine. Silicon star. Helium and neon deficient. Bluest known peculiar A-star: color,S:characteristic of about B4V. Classified A0p because He weak, but in other respects the color is more indicative of the,S:temperature than the spectral class of Ap stars. One of the hottest Ap stars known, about 17000K.,SB:Double lines.,VAR:Alpha CV 5.35 - 5.41V, 2.4660d. Spectrum var. same period.
HR 1733			BD+44 1170	34498	40242						05 20 02.3	+44 25 32	6.62 R	K0
HR 1734		18	BD+33 1010	34499	57893				3893		05 19 23.6	+33 59 08	6.49	A7V	5.3	3.8
HR 1736			BD+46 998	34533	40251				3903		05 20 39.3	+46 57 50	6.54	GIII+A2V	2.9	23.2	D:Fixed. Companion spectral class A.
HR 1738			BD+40 1253	34557	40248						05 20 14.8	+41 05 10	5.52	A3V
HR 1740		19	BD+33 1013	34578	57906	2399				1925	05 20 00.9	+33 57 29	5.03	A5II
HR 1749	ρ	20	BD+41 1162	34759	40269	2400					05 21 48.4	+41 48 16	5.23	B3V			G:Cas-Tau OB1.,SB:35.5d, K 28k/s, V0 +19k/s, asini 13.7.
HR 1752			BD+29 869	34790	77124						05 21 12.7	+29 34 12	5.76 R	A1V s	0.4	0.0	SB:6.2, 6.6v, sep. 0.0005", 2.1517d, K 113.3k/s, V0 -19.7k/s, msin3i 1.71, asini 3.35; vsini both components 53k/s.
HR 1760			BD+40 1268	34904	40290						05 22 50.3	+41 01 46	5.54	A3V
HR 1768		22	BD+28 788	35076	77139						05 23 22.9	+28 56 12	6.46	B9V s
HR 1773	σ	21	BD+37 1175	35186	57981		I		3984		05 24 39.2	+37 23 08	4.99	K4III	7.0	8.7	D:AB fixed.
HR 1775			BD+31 954	35238	57987						05 24 38.3	+31 13 26	6.28	K1III
HR 1776			BD+31 955	35239	57988						05 24 38.5	+31 08 35	5.94	B9III
HR 1779			BD+34 1031	35295	57999				4000 A		05 25 13.0	+34 51 19	6.55	K1pIII-IV+F6V	1.8	31.2	D:CPM. Companion F6V.,S:Component A has abnormally strong CN. Lambda 4150 star.
HR 1794			BD+35 1102	35519	58029	2408	I				05 26 54.3	+35 27 26	6.15	K2			G:Open cluster NGC 1907 #1.
HR 1795			BD+34 1040	35520	58028						05 26 48.9	+34 23 30	5.94	A0III			S:Also classified A1p.
HR 1796			BD+33 1045	35521	58030						05 26 51.3	+33 15 46	6.15	K0
HR 1804			BD+30 898	35600	58040						05 27 08.3	+30 12 31	5.74	B9Ib			G:Aur OB1. Concentration of hydrogen emission in direction of this association.
HR 1805	φ	24	BD+34 1048	35620	58051		I	W			05 27 38.9	+34 28 33	5.07	K3IIICN+2	3.2	206.8	G:Hyades group.
HR 1822			BD+29 909	35984	77205						05 29 40.6	+29 11 11	6.24	F6III
HR 1824			BD+41 1206	36040	40387	2412					05 30 48.6	+41 27 43	6.00	K0IIIp			S:Lambda 4150 star.
HR 1825			BD+39 1322	36041	58129			W			05 30 45.1	+39 49 33	6.37	G9III	1.3	75.4	D:Companion 7.62V, +0.94(B-V), +0.69(U-B), G8III.
HR 1843	χ	25	BD+32 1024	36371	58164	1151					05 32 43.7	+32 11 31	4.76	B5Iab			G:Aur OB1. Concentration of hydrogen emission in direction of this association.,SB:655.16d, K 20.5k/s, V0 -0.2k/s, asini 182.
HR 1846			BD+41 1218	36404	40426						05 33 28.7	+42 06 32	6.55	B9IIIp:Hg:
HR 1850			BD+32 1028	36484	58179						05 33 27.5	+32 48 04	6.48	A2m
HR 1854			BD+34 1083	36499	58182						05 33 38.0	+34 43 33	6.27	A3IV
HR 1866			BD+54 914	36678	25276	2416	I				05 36 35.2	+54 25 44	5.73	M0III
HR 1869			BD+47 1178	36719	40466	2417					05 36 15.9	+47 42 55	6.11	dF0
HR 1884			BD+40 1346	36891	40481						05 36 52.4	+40 10 56	6.09	G3Ib+F
HR 1904			BD+33 1102	37138	58263						05 37 45.7	+33 33 33	6.33	K0
HR 1914		26	BD+30 963	37269	58280				4229	2485	05 38 38.1	+30 29 33	5.40	F9III+B9.5V	0.3	0.2	D:AB 6.0 G5III, 6.3 A2V, 53.2y, a = 0.135". Combined, mag., colors. C, 8.57V, +0.28(B-V), +0.09(U-B), F0V at 12",,D:physical; D, 11.5v at 33". Resolved by speckle interferometry 1983.93, sep. 0.12".
HR 1924			BD+29 947	37367	77354						05 39 18.4	+29 12 55	5.96	B2IV-V	2.0	0.0	G:Cas-Tau OB1.,SB:6.2, 8.2, sep. 0.00001", about 6.5d, K 9k/s.
HR 1925			BD+53 934	37394	25319			W			05 41 20.3	+53 28 52	6.23	K1V	2.8	688.0	D:Component B, 9.9v M1 at 99", is BD +53d935, CPM. Component D is F5. Other companions 12.4 and 12.8v.
HR 1938			BD+31 1048	37519	58319	2425				2537	05 40 35.9	+31 21 29	6.04	B9.5III-IVp:
HR 1939			BD+31 1049	37536	58322		I			NO Aur	05 40 42.1	+31 55 15	6.11	M2IIIS			G:Aur OB1.,VAR:Lc 6.13 - 6.30V.
HR 1945			BD+29 953	37646	77393				4262 A		05 41 21.0	+29 29 15	6.43	B8IV	0.4	26.1	D:CPM, B is 7.18V, -0.04(B-V), -0.14(U-B), B9.5V, vsini 120k/s.,SB:ADS 4254A.
HR 1971	ο	27	BD+49 1398	38104	40583	216					05 45 54.0	+49 49 35	5.47	A2VpCr			G:UMa stream.
HR 1974			BD+40 1403	38189	40584						05 45 49.5	+40 30 26	6.58	A3Del Del
HR 1979			BD+42 1396	38358	40609	2431					05 47 14.7	+42 31 36	6.29	K0
HR 1995	τ	29	BD+39 1418	38656	58465		I		4398		05 49 10.5	+39 10 52	4.52	G8IIIFe-1	6.1	49.6	G:Ursa cluster? UMa stream.
HR 2003			BD+51 1117	38765	25411	2437					05 50 56.4	+51 30 53	6.29	K1III
HR 2011	υ	31	BD+37 1336	38944	58496	2440	I			2661	05 51 02.4	+37 18 20	4.74	M0+III-IIIbFe-0.5			VAR:Amp. 0.1V. Cycles 35-36d in 1970-1 not confirmed in other seasons.
HR 2012	ν	32	BD+39 1429	39003	58502	221	I		4440		05 51 29.4	+39 08 55	3.97	G9.5III*	7.3	54.6	D:Companion optical.,S:G9.5III CN 0.5 Fe 1 Ba 0.2:
HR 2018			BD+32 1109	39045	58504		I		4443	Var	05 51 25.7	+32 07 30	6.25	M3III v	5.9	15.2	M:High space velocity.,S:Spectrum may be variable.,VAR:Amp. 0.10V.
HR 2025			BD+39 1435	39182	58524						05 52 39.5	+39 34 28	6.45 R	A2V
HR 2028			BD+33 1179	39225	58528	2443	I			2681	05 52 40.1	+33 55 03	5.98	M1.5II-III			M:High space velocity.
HR 2029	ξ	30	BD+55 1027	39283	25450	1157					05 54 50.8	+55 42 25	4.99	A2V			G:Sirius group?,N:Flamsteed also called this star 32 Cam = 30 Aur.,R:Radius relative to Sun = 2.6.,S:Lambda Boo type.
HR 2045			BD+51 1128	39551	25467						05 56 14.4	+51 48 14	6.49 R	A5V
HR 2046			BD+31 1139	39586	58569						05 54 59.0	+31 42 06	5.90	A5IV
HR 2054			BD+49 1423	39743	40720						05 57 04.9	+49 01 46	6.47	G8III
HR 2066			BD+28 952	39866	77744						05 56 33.8	+28 56 32	6.32	A2II
HR 2077	δ	33	BD+54 970	40035	25502	225	I	W			05 59 31.6	+54 17 05	3.72	K0-III	5.8	115.4
HR 2079			BD+55 1036	40062	25504						05 59 45.7	+55 19 15	6.44	A5m
HR 2080			BD+54 971	40083	25505						05 59 48.1	+54 32 50	6.14	K2III
HR 2081			BD+49 1428	40084	40743						05 59 21.8	+49 55 28	5.89	G5III			SB:219.13d, K1 32.2k/s, K2 33.23k/s, V0 -4.09k/s, a1sini 97.1, a2sini 100.1.
HR 2088	β	34	BD+44 1328	40183	40750	227	I		4556	Bet Aur	05 59 31.7	+44 56 51	1.90	A2IV	8.9	184.6	D:AB binary. C, 14.1v at 13".,G:In Ursa cluster; Sirius group; UMa stream; UMa cluster.,N:Menkalinan; Menkalina.,R:Radius relative to Sun = 3.0.,SB:ADS 4556A, 3.9600d, K 107.5k/s, V0 -17.1k/s, msin3i 2.20, asini 5.85. Masses 2.33, 2.25 solar. Rotational,SB:velocities both components <30k/s. Second SB ever discovered, by Antonia Maury, 1889.,VAR:ADS 4556A, EA 1.89 - 1.98V, 1.93 - 2.02B, A2+A2, 3.9600421d, i 78.5d.
HR 2091	π	35	BD+45 1217	40239	40756		I			Pi Aur	05 59 56.1	+45 56 13	4.26	M3II e			C:Large infrared excess.,M:Radio star.,S:Ultraviolet FeII emission.,VAR:Lc 4.24 - 4.34V. Radio emission at 2.85cm indicates mass loss.
HR 2095	θ	37	BD+37 1380	40312	58636		I		4566	The Aur	05 59 43.3	+37 12 45	2.62	A0pSi	4.5	3.5	D:AB binary , combined mag., colors. B is 7.2v G2V. C, 11v at 49" optical.,DYN:0.032".,R:Radius 3.3 solar.,VAR:ADS 4566B. Alpha CV 2.62 - 2.70V. Amp. 0.43m at 1400A, 1.3735d. Magnetic field varies 3.618d.
HR 2096			BD+44 1332	40325	40769				4576		06 00 19.0	+44 35 31	6.22	K2III+K0III	4.0	34.2	D:AB probably binary. B, 11v at 2". Component C, K0III, optical.
HR 2101		36	BD+47 1227	40394	40778						06 00 58.6	+47 54 07	5.73	B9.5pSiFe
HR 2105			BD+48 1333	40486	40789	2458	I				06 01 43.1	+48 57 34	5.96	K0
HR 2110			BD+31 1164	40588	58657						06 01 10.2	+31 02 05	5.98 R	A2V
HR 2112			BD+49 1441	40626	40801						06 02 48.7	+49 54 20	6.05	B9.5IV
HR 2115			BD+43 1421	40722	40808						06 02 53.6	+43 22 43	6.42 R	K0
HR 2119		38	BD+42 1473	40801	40818	2461					06 03 18.0	+42 54 42	6.10	K0II			G:Sigma Pup group.
HR 2122			BD+32 1166	40832	58688						06 02 55.1	+32 38 09	6.24	F4V
HR 2123			BD+51 1146	40873	25548	2463			4633	2804	06 04 29.1	+51 34 24	6.45	A7III	2.8	39.0	D:BC, 9.0, 10.0v, sep. 0.6", CPM with A.,VAR:Delta Sct?
HR 2132		39	BD+42 1477	41074	40840					2812	06 05 03.4	+42 58 54	5.87	F3V			G:Hyades group.
HR 2137			BD+37 1405	41162	58716				4649		06 05 02.6	+37 57 51	6.34	K0III+A2	5.6	17.9	D:Confusion as to whether B or C is the brighter, B at 18", C at 84" from A.
HR 2139			BD+33 1236	41269	58727						06 05 34.0	+33 35 57	6.23	B9pSi
HR 2141			BD+35 1334	41330	58739			W			06 06 08.5	+35 23 15	6.12	G0V	3.4	122.0
HR 2143		40	BD+38 1377	41357	58749	2465				Var?	06 06 35.1	+38 28 58	5.36	A4m			SB:28.28d, K 51.4k/s, V0 +16.9k/s, msin3i 1.35, asini 16.6.,VAR:Suspected of 0.01m variability.
HR 2146			BD+29 1112	41429	77958		I		4673		06 06 22.5	+29 30 45	6.08	M3II+F7V	5.0	10.0	D:CPM. Companion 10.72V, +0.90(B-V), +0.25(U-B), F7V.
HR 2147			BD+41 1357	41467	40868						06 07 26.9	+41 51 15	6.12	K0III
HR 2153			BD+41 1365	41636	40881						06 08 23.0	+41 03 20	6.36	G9III
HR 2172			BD+52 1041	42083	25613						06 11 46.0	+52 38 50	6.30	A5IIIm			SB:106d, K 40.5k/s, V0 +13.5k/s, msin3i 1.55, asini 45.8; vsini both components 30k/s. Unresolved by speckle,SB:interferometry.
HR 2175		41	BD+48 1352	42126	40924				4773 B		06 11 36.5	+48 42 47	6.82 H	A8V	0.8	7.7	D:Binary with HR 2176.,G:Hyades group.
HR 2176		41	BD+48 1352	42127	40925				4773 A		06 11 36.6	+48 42 40	6.09 H	A3V	0.8	7.7	D:Binary with HR 2175.,G:Hyades group.
HR 2188			BD+51 1163	42466	25630						06 13 45.3	+51 10 21	6.04	K1III
HR 2189			BD+32 1217	42471	58852	2470	I				06 12 20.1	+32 41 36	5.78	M2IIIa
HR 2217			BD+36 1388	43017	58905	1167			4849 A		06 15 39.0	+36 08 55	6.92	F4IV	0.6	11.3	D:AB CPM. B is dF0; C 12.3v at 202" optical. D, 11.5v at 120" from A.
HR 2219	κ	44	BD+29 1154	43039	78143	1168	I			2877	06 15 22.7	+29 29 53	4.35	G8.5IIIb
HR 2228		42	BD+46 1122	43244	40999						06 17 34.7	+46 25 27	6.52	F0V			G:UMa stream.
HR 2239		43	BD+46 1124	43380	41010						06 18 16.9	+46 21 38	6.38	K2III			G:Eta Cep group.
HR 2264		45	BD+53 1008	43905	25681	2484					06 21 46.1	+53 27 08	5.36	F5III			SB:6.5013d, K 31.7k/s, V0 -1.5k/s, asini 2.83.
HR 2272			BD+29 1190	44092	78259						06 21 12.1	+29 32 28	6.43	A1V s
HR 2289	ψ¹	46	BD+49 1488	44537	41076	242	I			Psi1 Aur	06 24 53.9	+49 17 17	4.91	K5-M0Iab-Ib			VAR:Lc? 4.75 - 5.70V, 6.6 - 7.2p.
HR 2297			BD+29 1213	44766	78333						06 24 52.6	+29 42 26	6.71	B8IIIn
HR 2314			BD+47 1299	45105	41109						06 27 51.1	+47 24 19	6.56	A0V
HR 2319			BD+32 1300	45192	59096						06 27 35.5	+32 33 47	6.43	K0
HR 2332		48	BD+30 1238	45412	59128					RT Aur	06 28 34.1	+30 29 35	5.55	F8Ib v			S:Also classified F4Ib-G1Ib.,VAR:CDelta 5.02 - 5.82V. Per. changing, 3.728365 before 1950, 3.728115 since. CaII emission on rising branch of light,VAR:curve. Blue companion suspected.
HR 2338		47	BD+46 1149	45466	41130	2496	I				06 30 03.0	+46 41 08	5.90	gK4
HR 2372			BD+32 1324	46052	59194	2500				WW Aur	06 32 27.2	+32 27 17	5.87	A3m+A3m:			S:Also classified A3m: + A3m:,SB:2.5250d, K 115.6k/s, V0 -8.7k/s, msin3i 1.98, asini 4.01. Masses 1.92, 1.90 solar. vsini same for both,SB:components 35k/s.,VAR:EA 5.79 - 6.54V, 2.52501922d. Per. changes. Rot. line apsides per. about 40,000d.
HR 2383			BD+33 1356	46251	59222						06 33 42.7	+33 01 27	6.42 R	A3V
HR 2398		49	BD+28 1168	46553	78524	2504				3032	06 35 12.1	+28 01 20	5.27	A0Vnn
HR 2405			BD+38 1539	46687	59280		I	W		UU Aur	06 36 32.9	+38 26 43	5.29	C5II	5.6	17.9	S:Infrared spectra show CO, CN and C2 molecules.,VAR:SRb 7.83 - 10.00B, 8.2 - 10.0p, 234d. Mean mag. varies in per. about 3500d.
HR 2419		51	BD+39 1690	47070	59316	250	I				06 38 39.5	+39 23 27	5.69	K5III			G:Hyades group.
HR 2420	ψ³	52	BD+40 1665	47100	59319						06 38 49.2	+39 54 09	5.20	B8III
HR 2425		53	BD+29 1293	47152	78571			D			06 38 23.0	+28 59 03	5.79	B9npEu	0.0	0.1	D:Discovered by both occultation and speckle interferometry 1978, sep. 0.075"; 1983.93, sep. 0.13".,S:Spectra show Hg 4077; Eu, Cr enhanced. Overabundant elements are V by factor of 300; Sr by 1500; Y by 100 and rare,S:earths by hundreds of thousands.
HR 2427	ψ²	50	BD+42 1585	47174	41239		I	W			06 39 19.9	+42 29 20	4.79	K3III	5.5	52.1
HR 2434			BD+44 1506	47270	41245						06 39 58.0	+44 00 50	6.41 R	K1III
HR 2438		54	BD+28 1196	47395	78593				5289	3065	06 39 33.1	+28 15 47	6.03	B7III	1.6	0.8
HR 2452			BD+36 1482	47703	59365	2516					06 41 37.7	+35 55 55	6.46	F8III
HR 2459	ψ⁴	55	BD+44 1518	47914	41288	2517	I				06 43 05.0	+44 31 28	5.02	K5III
HR 2464			BD+37 1567	48073	59406						06 43 13.8	+37 08 49	6.19	K0
HR 2471			BD+36 1494	48272	59425						06 44 12.6	+36 06 35	6.31 R	A2V
HR 2483	ψ⁵	56	BD+43 1595	48682	41330	255			5425		06 46 44.3	+43 34 39	5.25	G0V	3.4	36.2	D:Companion orange, optical.
HR 2487	ψ⁶	57	BD+48 1436	48781	41346	1176	I				06 47 39.6	+48 47 22	5.22	K0III
HR 2516	ψ⁷	58	BD+41 1536	49520	41380	2527	I	W			06 50 45.9	+41 46 53	5.02	K3III	5.0	40.9	G:61 Cyg group.
HR 2532			BD+45 1359	49949	41406						06 53 07.6	+44 50 22	6.26	A8Vn
HR 2539		59	BD+39 1771	50018	59571				5534	OX Aur	06 53 01.5	+38 52 09	6.12	F2VDel Del v	3.9	22.3	D:AB fixed.,M:Space motion almost identical to that of the Sun.,S:Also classified A7n-F3IV.,VAR:Delta Sct 5.94 - 6.14V, primary period 0.115442, secondary 0.154412d.
HR 2541		60	BD+38 1636	50037	59576			S			06 53 13.4	+38 26 17	6.30	dF5			N:Sometimes this star, sometimes HR 2547 have been called Psi8 Aur. To avoid future confusion this designation,N:is abandoned for both.
HR 2542			BD+35 1511	50056	59574		I			3250	06 53 03.4	+35 47 19	6.01	K3III:
HR 2547	ψ⁸	61	BD+38 1638	50204	59589						06 53 57.0	+38 30 18	6.48	B9.5pSi			N:See note for HR 2541.,S:Hg, Mn.
HR 2556			BD+46 1202	50384	41426						06 55 15.2	+45 49 35	6.34	K0III-IV			G:Hyades group.
HR 2557			BD+44 1551	50420	41429					V352 Aur	06 55 14.7	+43 54 36	6.13	A9III			VAR:Delta Sct 6.037 - 6.054y. About 4 hrs. One of most luminous Delta Sct stars: abs. mag. about 0.0V.
HR 2568	ψ⁹		BD+46 1203	50658	41446					Var?	06 56 32.3	+46 16 27	5.87	B8IIIe			S:Shell star.,VAR:Emission var. about 16 yrs.
HR 2573			BD+46 1205	50763	41450						06 56 56.0	+46 42 18	5.86	gK0
HR 2600		62	BD+38 1656	51440	59658	2538	I				06 59 02.8	+38 03 08	6.00	K2III
HR 2675			BD+37 1660	53925	59812						07 08 36.3	+37 26 42	6.16	K1III
HR 2696		63	BD+39 1882	54716	59866	274	I				07 11 39.3	+39 19 14	4.90	K4III-IIIa
HR 2753		64	BD+41 1630	56221	41679	276					07 18 02.2	+40 53 00	5.78	A5Vn			G:In Ursa cluster?
HR 2775			BD+42 1699	56941	41705						07 21 03.1	+42 39 20	6.35	K0
HR 2792			BD+39 1927	57263	60012						07 22 13.4	+38 59 46	6.40	K0
HR 2793		65	BD+37 1707	57264	60010	2568	I		6009		07 22 02.6	+36 45 38	5.13	K0III	5.5	11.4	D:AB CPM. C, 12.7v at 42" optical.
HR 2805		66	BD+40 1852	57669	41738	1191	I				07 24 08.5	+40 40 20	5.19	K1+IIIaCN1

Legende

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)

Kataloge

Auriga / Yale Bright Star Catalog (HR)

Legende

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