Catalogues

Catalogue

Constellation

Leo / 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 3723			BD+25 2088	80956	80797						09 23 31.8	+25 10 59	6.41	G5IV
HR 3731	κ	1	BD+26 1939	81146	80807	1244	I		7351	4478	09 24 39.3	+26 10 56	4.46	K2III	5.1	2.5	D:AB binary.,N:Al Minliar al Asad.,VAR:NSV 4478 is ADS 7351B, 9.5 - 11.5v.
HR 3736			BD+17 2078	81361	98561	2750					09 25 32.5	+16 35 08	6.29	gG9
HR 3754	ω	2	BD+09 2188	81858	117717				7390		09 28 27.5	+09 03 24	5.41	F9V	0.7	0.5	D:5.87 dF8, 6.53, 116.85y, a = 0.875" or 118.227y, a = 0.880".,DYN:0.024".,SB:116.85y D, K 2.2k/s, V0 -6.0k/s, asini 1070. Orbit questioned by Morbey and Griffin (1987, ApJ, 317, 343).
HR 3755		3	BD+08 2226	81873	117718	2752			7391		09 28 29.2	+08 11 18	5.71	K0III	5.3	25.2	D:CPM.
HR 3773	λ	4	BD+23 2107	82308	80885	2756	I			4514	09 31 43.2	+22 58 05	4.31	K5III v			N:Alterf.,VAR:Sp. var., 7 - 12d.
HR 3779		6	BD+10 2014	82381	117751		I		7416		09 31 57.6	+09 42 57	5.07	K2.5IIIbFe-0.5	4.4	37.3	D:Companion 9.54V, +0.44(B-V), +0.03(U-B), F6V.,SB:ADS 7416A. Sp. comp. B, F5.
HR 3782	ξ	5	BD+11 2053	82395	98627	1246	I	D		4518	09 31 56.7	+11 17 59	4.97	K0-III-IIIb	1.9	0.0	D:Suspected occultation double.,SB:Suspected SB, 5.3, 7.2, sep. 0.0066".
HR 3792			BD+29 1913	82523	80900	2760			7426		09 33 18.3	+28 22 05	6.53	A3Vnn	5.2	30.5	D:Optical.
HR 3804			BD+24 2104	82670	80909		I				09 33 59.1	+23 27 14	6.25	gK7
HR 3818		7	BD+15 2077	83023	98662				7448 A		09 35 52.9	+14 22 47	6.36	A1V	3.2	41.2	D:CPM. Companion F8V. Discordant magnitudes and colors: Nicolet: A = 7.86V, -0.10(B-V), -0.43(U-B); B = 9.07V,,D:+0.55(B-V), +0.01(U-B). USNO Photoelectric Catalogue: A = 6.36V, +0.01(B-V), +0.03(U-B); B = 9.51V, +0.50(B-V),,D:+0.03(U-B). Component A suspected occultation double.
HR 3820			BD+31 2011	83069	61594	2765	I			4545	09 36 42.9	+31 09 42	5.56	M2IIIa
HR 3826		8	BD+17 2109	83189	98673	2766	I	D			09 37 02.6	+16 26 16	5.69	gK1			D:Suspected occultation double; possibly SB.
HR 3827		10	BD+07 2160	83240	117807	2767	I			4551	09 37 12.7	+06 50 09	5.00	K1III v
HR 3850			BD+31 2026	83787	61633		I	W		DR Leo	09 41 35.2	+31 16 41	5.89	K6III	7.5	28.4	VAR:Lb 5.84 - 5.98V.
HR 3852	ο	14	BD+10 2044	83808	98709	365	I		7480		09 41 09.0	+09 53 32	3.52	F6II+A1-5V	0.2	0.0	D:Component B, 9.9v at 85".,N:Subra.,SB:ADS 7480A, 14.4980d, K 54.1k/s, V0 +27.1k/s, msin3i 1.30, asini 10.8. Unresolved by speckle interferometry.,SB:vsini both components =<50k/s.
HR 3853		13	BD+26 1991	83821	80970						09 41 38.5	+25 54 46	6.24	gK2
HR 3861		15	BD+30 1901	84107	61656	1251					09 43 33.3	+29 58 28	5.64	A2IV
HR 3866	ψ	16	BD+14 2136	84194	98733	1252	I	W		4594	09 43 43.9	+14 01 18	5.35	M2IIIab	5.3	281.8
HR 3869			BD+19 2251	84252	98742			W			09 44 30.0	+18 51 49	6.50 R	K0	6.0	31.2
HR 3873	ε	17	BD+24 2129	84441	81004	367	I			4613	09 45 51.1	+23 46 27	2.98	G1II			N:Ras Elased Australis; Al Ras al Asad al Janubiyyah; Algenubi; with HR 3905, Al Ashfar.,VAR:Cep amp. 0.1V, period a few days.
HR 3876			BD+07 2181	84542	117898	2781	I				09 46 10.0	+06 42 31	5.79	M1.5IIIab			G:Wolf 630 group.
HR 3877		18	BD+12 2090	84561	98755		I				09 46 23.3	+11 48 36	5.63	gK4
HR 3880		19	BD+12 2095	84722	98767			S			09 47 25.9	+11 34 06	6.45	A7Vn	0.2	0.0	D:Binary 7.0, 7.2v, sep. 0.031", resolved by speckle interferometry at 4-meter Mayall telescope, but unresolved 1983.96,D:at Pic du Midi. Combined mag., colors.
HR 3882			BD+12 2096	84748	98769		I			R Leo	09 47 33.5	+11 25 44	6.02	M8IIIe v			C:R-I corresponds to 7.52V, +1.41(B-V), +0.28(U-B).,G:Wolf 630 group.,P:Polarization possibly due to circumstellar dust scattering.,R:Speckle interferometer observations show abrupt variations in diameter as a function of wavelength, interpreted as due,R:to large opacity of TiO. 0.032" at 5400A to 0.054" at 7300A to 0.030" at 7400A. Occultation diam. = 0.067", the,R:largest measured angular diameter of any star other than the Sun.,S:SiO maser. H2O bands. Silicate emission. Also classified M6e-M9.5IIIe.,VAR:M 4.4 - 11.3v, 309.95d. Period varies from 307.4 to 317.8d. Discovered by Koch in 1782.
HR 3889		20	BD+21 2113	85040	81035	2785		W		DG Leo	09 49 50.1	+21 10 46	6.09	A7IVn	0.3	0.3	D:AB, about 200y. B also A8IV.,S:Sr enhanced. Also classified A8IVs and F0IIIn.,SB:Comp. A of visual double, 4.1467d, K 101.2k/s, V0 +27.2k/s, msin3i 1.80, asini 5.77. Both components A8IV. Could,SB:be eclipsing. Nearly equal masses. Secondary vsini 30k/s.,VAR:Comp. B of visual double, Delta Sct 6.08 - 6.12V, 0.08184505d.
HR 3896		23	BD+13 2164	85268	98809		I				09 51 02.0	+13 03 58	6.46	M0III
HR 3900		22	BD+25 2169	85376	81054						09 51 53.0	+24 23 43	5.32	A5IV			G:Wolf 630 group.
HR 3905	μ	24	BD+26 2019	85503	81064	371	I				09 52 45.8	+26 00 25	3.88	K2IIICN1Ca1			N:Ras Elased Borealis; Rasalas; Ras al Asad al Shamaliyy; Alshemali; with HR 3873, Al Ashfar.,S:Super metal-rich star.
HR 3926			BD+09 2262	86080	118001	2794					09 56 26.0	+08 55 59	5.85	gK2
HR 3936			BD+28 1824	86358	81120						09 58 26.1	+27 45 32	6.30 R	F3V			SB:Secondary vsini 30k/s.
HR 3937	ν	27	BD+13 2183	86360	98876	2800					09 58 13.4	+12 26 41	5.26	B9IV
HR 3938			BD+09 2269	86369	118023		I				09 58 07.6	+08 18 51	6.04	gK3
HR 3942			BD+30 1946	86513	81129	2803					09 59 36.2	+29 38 43	5.73	gG9
HR 3950	π	29	BD+08 2301	86663	118044	378	I			4699	10 00 12.8	+08 02 39	4.70	M2-IIIab e			R:Occultation diam. = 0.0052 - 0.0059".,S:Ultraviolet FeII emission.,VAR:Amp. 0.10V.
HR 3952			BD+22 2164	87015	81154	2807					10 02 48.9	+21 56 57	5.66	B2.5IV
HR 3969			BD+16 2077	87500	98944						10 05 40.9	+15 45 27	6.37	F2Vn
HR 3975	η	30	BD+17 2171	87737	98955	379		W		4738	10 07 20.0	+16 45 46	3.52	A0Ib	0.5	0.1	D:Binary, sep. 0.097", unresolved by speckle interferometry 1982.17.,G:Sco-Cen assoc.,S:Large helium abundance due to chromospheric shell. Metal abundance greater than in Sun.
HR 3980		31	BD+10 2112	87837	98964		I		7649		10 07 54.3	+09 59 51	4.37	K3.5IIIbFe-1	7.7	7.9	D:CPM.,R:Occultation diam = 0.0028 - 0.0031".
HR 3982	α	32	BD+12 2149	87901	98967	380	I		7654 A	4750	10 08 22.3	+11 58 02	1.35	B7V e	6.8	177.6	C:Color excess E(B-V) = +0.01.,D:AB binary, B, 8.13V, +0.86(B-V), +0.51(U-B), K1V. BC, 7.6, 13.1v, 2000y, a = 4.163".,N:REGULUS; Cor Leonis; Rex; Al Kalb al Asad; Kabeleced.,R:Diam. = 0.00132 - 0.00137".,S:C1 neutral carbon continuum shows discontinuities in UV. Excess IR emission.
HR 3998		34	BD+14 2217	88355	98991				7674		10 11 38.2	+13 21 18	6.44	F7V	0.8	0.2	D:CPM.,G:Sirius group; UMa stream.
HR 4006			BD+27 1862	88639	81243						10 13 49.8	+27 08 09	6.04	G3IIIFe-1			G:61 Cyg group.
HR 4012			BD+21 2165	88737	81250						10 14 29.7	+21 10 04	6.02	F9V
HR 4028			BD+18 2338	88987	99032				7704		10 16 16.1	+17 44 25	6.55 R	A9IV	0.3	1.1	D:7.2 dF2, 7.5, 552.0y, a = 1.299" or 810.5y, a = 1.198". Combined mag.
HR 4030		35	BD+24 2207	89010	81260		I				10 16 32.3	+23 30 11	5.97	G1.5IV-V
HR 4031	ζ	36	BD+24 2209	89025	81265	384	I	W		4804	10 16 41.4	+23 25 02	3.44	F0III	2.3	325.9	D:Primary unresolved by speckle interferometry 1982.17.,G:Sirius group; UMa stream.,N:Adhafera; Aldhafara; Aldhafera.
HR 4032			BD+26 2064	89024	81264						10 16 41.9	+25 22 17	5.84	gK2
HR 4035		37	BD+14 2228	89056	99034	2824	I				10 16 40.7	+13 43 42	5.41	M1.5IIIab
HR 4039		39	BD+23 2207	89125	81270				7712		10 17 14.6	+23 06 22	5.82	F8Vb w	6.0	7.6	D:Companion is M1.,DYN:0.028".
HR 4041			BD+28 1867	89239	81278						10 18 10.3	+27 24 55	6.52	A0V
HR 4048			BD+25 2231	89344	81285						10 19 00.7	+24 42 42	6.40 R	K0
HR 4054		40	BD+20 2466	89449	99065					4822	10 19 44.1	+19 28 15	4.79	F6IV			VAR:Delta Sct?, 4.77 - 4.83V.
HR 4057	γ¹	41	BD+20 2467	89484	81298		I		7724 A	4823	10 19 58.3	+19 50 30	2.61	K1-IIIbFe-0.5	1.2	4.5	D:AB 2.22 K0IIIP, 3.47 G7III, 618.56y, a = 2.505". B is HR 4058. Colors for combined light. Mag. for blend, 1.90V.,D:Component C is the flare star AD Leo (8.07-11.00B) at 5', optical.,DYN:0.013".,G:Gamma Leo group.,N:ALGIEBA; Algeiba; Al Gieba.,VAR:Originally confused with eclipsing star Y Leo when var. suspect number 6777 was assigned in 1965. Now HR 4057 is again,VAR:suspected of variability, 1.84 - 2.03V for combined HR 4057/8. Uncertain which component is the variable.
HR 4058	γ²	41	BD+20 2467	89485	81299		I		7724 B	4823	10 19 58.6	+19 50 26	3.80 H	G7IIIFe-1	1.2	4.5	D:See HR 4057.,DYN:0.013".,G:Gamma Leo group.,VAR:See HR 4057.
HR 4070		42	BD+15 2192	89774	99080					4828	10 21 50.3	+14 58 32	6.12	A1V			VAR:Probably not var. Comparison star was variable.
HR 4077		43	BD+07 2289	89962	118269						10 23 00.4	+06 32 33	6.07	K3III			G:Wolf 630 group.
HR 4088		44	BD+09 2351	90254	118286	2835	I			DE Leo	10 25 15.2	+08 47 05	5.61	M3IIIabs			VAR:SRb? 5.60 - 5.67V, 1 - 2d?
HR 4097			BD+20 2487	90472	99128	2837					10 27 00.5	+19 21 52	6.15	K0
HR 4101		45	BD+10 2152	90569	99136				7781	CX Leo	10 27 39.0	+09 45 45	6.04	A0pSiCr:	6.3	37.2	D:Primary is occultation double, 6.7, 6.7v, sep. 0.02".,S:Magnetic star. Also classified B8.5Vp.,SB:12,658.4d, K 11.0?k/s, V0 -7.8k/s, asini 1650.,VAR:Alpha CV 5.97 - 6.15V, 7.897d. Magnetic var. 7.9d? and var. Sr, Cr.
HR 4127		46	BD+14 2255	91232	99172	1272	I			4883	10 32 11.8	+14 08 14	5.46	M1.5IIIbCa-1			R:Occultation diam. = 0.0056".
HR 4133	ρ	47	BD+10 2166	91316	118355	396		W		Rho Leo	10 32 48.7	+09 18 24	3.85	B1Ib	0.4	0.0	C:Color excess E(B-V) = +0.08.,D:4.4, 4.8v, sep. 0.11"; combined mag., colors.,M:Old disk population runaway star.,S:Lyman beta observed from COPERNICUS. Nitrogen enhanced, and carbon deficient.,SB:Inferred statistically by F. Schlesinger in 1915. Unresolved by speckle interferometry 1982.17.,VAR:Alpha Cyg 3.83 - 3.90V.
HR 4146		48	BD+07 2330	91612	118376	2846	I				10 34 48.0	+06 57 13	5.08	G8.5IIIFe-1Ca-1			S:Also classified G9III CN-1.5 Fe-1.
HR 4148		49	BD+09 2374	91636	118380				7837	TX Leo	10 35 02.2	+08 39 01	5.67	A2V	2.0	0.0	D:A is SB. Visual companion 8.5v at 2.4"; CPM.,SB:5.8, 7.8v, sep. 0.0005", 2.4451d, K 62.6k/s, V0 +16.7k/s, asini 2.10.,VAR:ADS 7837A, EA 5.66 - 5.75V, 2.4450566d.
HR 4197			BD+20 2514	92941	81496						10 44 14.5	+19 45 31	6.27	A5V
HR 4207			BD+07 2356	93244	118483	1278					10 46 05.7	+06 22 23	6.37	gK1			N:37 Sex in Leo.
HR 4208		51	BD+19 2371	93257	99281	1279	I				10 46 24.5	+18 53 29	5.49	gK3
HR 4209		52	BD+14 2294	93291	99282	2860					10 46 25.3	+14 11 41	5.48	gG4
HR 4227		53	BD+11 2283	93702	99305	409					10 49 15.4	+10 32 43	5.34	A2V
HR 4244			BD+01 2495	94180	118550			W			10 52 13.7	+01 01 31	6.38	A3V	5.8	39.2
HR 4245			BD+00 2710	94237	118555		I				10 52 36.1	-00 12 05	6.31	K5III			G:Wolf 630 group.
HR 4249			BD-01 2459	94363	137863				7967		10 53 24.9	-02 15 19	6.12	K0III+G0V	2.6	35.2	D:CPM. Companion 8.75V, +0.58(B-V), +0.01(U-B), G0V, RV = +18k/s.
HR 4253			BD-01 2460	94402	137871			W			10 53 43.7	-02 07 45	5.45	G8III			D:Suspected visual binary unresolved by speckle interferometry.,G:Hyades group.
HR 4259		54	BD+25 2314	94601	81583				7979 A		10 55 36.8	+24 44 59	4.50	A1V	1.9	6.5	D:Binary with HR 4260. Colors for combined light. Blended mag. 4.32V.
HR 4260		54	BD+25 2314	94602	81584				7979 B		10 55 37.3	+24 44 56	6.30 H	A2Vn	1.9	6.5	D:See HR 4259.
HR 4265		55	BD+01 2501	94672	118574				7982		10 55 42.4	+00 44 13	5.91	F2/3III/V	2.0	0.0	D:AB 6.1 F2III, 8.0, 128.34y, a = 0.823", or 90y, a = 0.75. Visual primary is SB, sep. 0.001".,DYN:0.030".,S:Also classified F3V.,SB:ADS 7982A.
HR 4267		56	BD+06 2369	94705	118576		I			VY Leo	10 56 01.5	+06 11 07	5.81	M5.5III v			S:Spectrum may be variable.,VAR:Lb? 5.69 - 6.03V.
HR 4269			BD+23 2279	94720	81589	2873	I				10 56 16.9	+22 21 06	6.14	K2
HR 4281			BD+12 2284	95216	99392	2877					10 59 41.1	+11 42 21	6.55	F5V
HR 4291		58	BD+04 2407	95345	118610	1284	I	D			11 00 33.6	+03 37 03	4.84	K1IIICN-0.5	0.0	0.1	D:Suspected occultation double.,S:BaII star?
HR 4294		59	BD+06 2384	95382	118615				8019		11 00 44.8	+06 06 05	4.99	A5III	7.5	44.8	D:Optical.
HR 4299		61	BD-01 2471	95578	137947	2879	I			5059	11 01 49.7	-02 29 05	4.74	M0IIIBa0.2
HR 4300		60	BD+20 2547	95608	81637	2880					11 02 19.8	+20 10 47	4.42	A1m
HR 4303			BD+00 2728	95771	137963			D			11 03 14.6	-00 45 09	6.14	F0V			D:Suspected occultation double.
HR 4306		62	BD+00 2729	95849	118634						11 03 36.6	-00 00 03	5.95	K3III
HR 4310	χ	63	BD+08 2455	96097	118648	418		W		5079	11 05 01.0	+07 20 10	4.63	F2III-IV v	4.3	276.4
HR 4319		65	BD+02 2387	96436	118668	1287			8060	5090	11 06 54.2	+01 57 20	5.52	G9IIICN-1	3.8	2.2	DYN:0.015".
HR 4322		64	BD+24 2318	96528	81681						11 07 39.7	+23 19 25	6.46	A5m			SB:40.45d, K 18k/s, V0 -2.9k/s, asini 9.96.
HR 4332		67	BD+25 2344	96738	81692	2889			8071		11 08 49.1	+24 39 30	5.68	A3IV	6.6	4.8
HR 4341			BD+15 2301	97244	99492						11 11 43.7	+14 24 01	6.30	A5V
HR 4356		69	BD+00 2761	97585	118731						11 13 45.6	-00 04 11	5.42	A0V
HR 4357	δ	68	BD+21 2298	97603	81727	422	I	W		5143	11 14 06.5	+20 31 25	2.56	A4V	6.0	191.4	G:Sirius group; UMa stream.,N:Zosma; Zozma; Zosca; Zozca; Duhr; Dhur; Zubra.,VAR:Delta Sct?
HR 4358			BD+08 2476	97605	118735	2895		W			11 14 01.8	+08 03 38	5.79	K3III	6.0	21.5	G:Wolf 630 group.
HR 4359	θ	70	BD+16 2234	97633	99512	423				5144	11 14 14.4	+15 25 46	3.34	A2V			N:Chort; Coxa; Chertan.
HR 4362		72	BD+23 2322	97778	81736	2897	I			5147	11 15 12.2	+23 05 44	4.63	M3IIb e			S:Ultraviolet FeII emission.,VAR:Lb?, 4.59 - 4.65V.
HR 4365		73	BD+14 2367	97907	99525		I	S			11 15 51.9	+13 18 27	5.32	K3III			D:If secondary is on main sequence, the spectral class is inferred to be F1V.
HR 4366			BD+13 2379	97937	99527						11 15 57.8	+12 50 41	6.67	A9Vp			S:Lambda Boo star, Mg 4481 wk.
HR 4368	φ	74	BD-02 3315	98058	138102	1292		W			11 16 39.7	-03 39 06	4.47	A7IVn	4.7	96.9	S:Shell star. Shell spectrum variable.
HR 4371		75	BD+02 2409	98118	118764	2902	I				11 17 17.4	+02 00 38	5.18	M0III-IIIb
HR 4378			BD+12 2319	98280	99544						11 18 21.0	+11 59 05	6.66	A2V
HR 4381		76	BD+02 2411	98366	118778						11 18 55.0	+01 39 02	5.91	gK0
HR 4386	σ	77	BD+06 2437	98664	118804	427					11 21 08.2	+06 01 46	4.05	B9.5V s
HR 4394			BD+00 2782	98960	118825		I				11 23 18.0	+00 07 54	6.05	K3
HR 4399	ι	78	BD+11 2348	99028	99587		I		8148	5184	11 23 55.5	+10 31 45	3.94	F4IV	2.8	1.1	D:4.03 F2IV, 6.70 G3V, 192.0y, a = 1.92"; possible subsystem with period about 16y. Combined mag., colors. Combined,D:mass about 3 Suns.,DYN:0.052".,G:UMa stream.,SB:192y, K 2.5k/s, V0 -11.0k/s, asini 2030. Orbit questioned by Morbey and Griffin (1987, ApJ, 317, 343).,VAR:Delta Sct?
HR 4400		79	BD+02 2418	99055	118831			D			11 24 02.3	+01 24 28	5.39	G8IIICN-0.5	0.7	0.0	D:Sep. 0.0034", discovered by occultation.
HR 4404			BD+12 2335	99196	99598	2912	I				11 24 58.9	+11 25 49	5.80	K4III			G:61 Cyg group.
HR 4408		81	BD+17 2356	99285	99601	2913		W			11 25 36.4	+16 27 23	5.57	F2V	3.6	55.7
HR 4410		80	BD+04 2463	99329	118851						11 25 50.0	+03 51 36	6.37	F3IV
HR 4414		83	BD+03 2502	99491	118864	1296			8162 A		11 26 45.3	+03 00 47	6.50	K0IV	1.1	28.5	D:AB 6.51 K0IV, 7.57 K2IV-V, >4000y. Combined mag. 6.16V. C, 9.9v at 90" probably physical.,DYN:0.032".,S:Both components UV deficient. 83 Leo A is a metal rich dwarf with high iron abundance.
HR 4418	τ	84	BD+03 2504	99648	118875	1297	I	W			11 27 56.2	+02 51 22	4.95	G7.5IIIa	2.6	91.1	G:Sirius group; UMa stream.
HR 4419			BD-00 2442	99651	138216			W			11 27 53.7	-01 42 00	6.25	gK2	1.4	0.3
HR 4426		85	BD+16 2266	99902	99629		I				11 29 41.9	+15 24 48	5.74	gK4
HR 4432		87	BD-02 3360	99998	138238	2917	I				11 30 18.9	-03 00 13	4.77	K3.5IIIFe-1			R:Occultation diam. = 0.0029 - 0.0037".
HR 4433		86	BD+19 2459	100006	99637	2918	I				11 30 29.0	+18 24 35	5.52	K0III			G:Probable Hyades group.
HR 4437		88	BD+15 2345	100180	99648				8196 A		11 31 44.9	+14 21 52	6.20	G0V	2.8	15.5	D:5500y. Circular orbit. Companion, K6IV.,DYN:0.046".,RV:ADS 8196B, -10k/s.
HR 4454			BD+11 2372	100518	99668						11 34 10.0	+11 01 25	6.55	A2m
HR 4455		89	BD+03 2521	100563	118929	2924					11 34 22.0	+03 03 36	5.77	F5V
HR 4456		90	BD+17 2374	100600	99673				8220		11 34 42.5	+16 47 49	5.95	B4V	1.1	3.6	D:AB binary. Combined mag., colors. B is B6. C, 9.64V F5 at 63".,SB:ADS 8220B.
HR 4459			BD+21 2331	100655	81886						11 35 03.8	+20 26 29	6.45	G9III
HR 4464			BD+11 2377	100740	99683	2927					11 35 43.4	+10 54 40	6.56	A4Vn
HR 4465			BD+28 2022	100808	81893				8231		11 36 17.9	+27 46 52	5.80	F0V	0.2	0.5	D:AB long period binary. C, 11.17V at 21" optical.,SB:ADS 8231A.
HR 4471	υ	91	BD-00 2458	100920	138298	437	I	D			11 36 56.9	-00 49 26	4.30	G8.5IIICN-0.5	4.5	0.1	D:Duplicity doubtful.
HR 4495		92	BD+22 2391	101484	81941	2936	I				11 40 47.1	+21 21 10	5.26	K1III
HR 4505			BD+23 2375	101688	81949						11 42 05.2	+22 12 39	6.59 R	F2IV-V
HR 4512			BD+26 2250	101980	81960	2940	I		8285		11 44 13.2	+25 13 06	6.02	K5III	4.7	36.7	D:Optical.
HR 4527		93	BD+21 2358	102509	81998	1304	I	W		DQ Leo	11 47 59.1	+20 13 08	4.53	G5III-IVe+A7V	4.4	74.3	S:H and K lines of the G-type component show moderately strong emission. Spectroscopic data indicate mag. of A component,S:is 5.52V, B component 5.09V.,SB:71.70d, K 23.7k/s, V0 -0.2k/s, asini 23.3. vsini of G-type component =<50k/s; of A-type, 110k/s.,VAR:RS, amp. 0.03V, 71.7d.
HR 4531			BD+15 2381	102590	99800				8311	5344	11 48 38.7	+14 17 03	5.88	F0V	2.4	1.1	D:6.0 A8V, 8.3 G2V, 122.0y, a = 0.68", 180y, a = 1.00". Combined mag., colors.,DYN:0.022".,G:Hyades moving group.,VAR:ADS 8311B, 7.5 - 9.5V.
HR 4534	β	94	BD+15 2383	102647	99809	444	I		8314	Bet Leo	11 49 03.6	+14 34 19	2.14	A3V	6.5	264.0	D:B, 15.7v at 40" physical; C, 13v at 80" optical.,N:DENEBOLA; Deneb Aleet.,R:Diam. = 0.00125 - 0.00133".,VAR:Delta Sct?, 2.09 - 2.16V.
HR 4535			BD+17 2402	102660	99812						11 49 14.9	+16 14 34	6.04	A3m			SB:2.7818d, K 31.0k/s, V0 -24.2k/s, asini 1.19.
HR 4543			BD+13 2465	102910	99827	2946			8320		11 50 55.3	+12 16 44	6.35	F0IVm s	4.9	14.9	G:Hyades moving group.,S:Also classified A5m.
HR 4564		95	BD+16 2319	103578	99869	1308		W			11 55 40.5	+15 38 48	5.53	A3V		90.	D:Discovered as double by W. Herschel, sep. 90" but no visual companion subsequently seen at that separation.,G:Possible Eggen group with HR 63, q.v.,SB:6.6254d, K 57.6k/s, V0 -20.4k/s, asini 5.25.

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

Leo / Yale Bright Star Catalog (HR)

Legend

References