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Serpens / 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 5654			BD+19 2935	134943	101429	3199	I	W		FL Ser	15 12 04.3	+18 58 33	5.89	M4IIIab	1.9	0.5	D:Resolved by speckle interferometry 1986.45, sep. 0.51".,VAR:Lb 5.79 - 6.02V.
HR 5659			BD+19 2939	135101	101437				9535 A		15 12 43.5	+19 17 09	6.68	G5V	0.8	23.7	D:Binary. Companion 7.53V, +0.35(R-I), dG6.,DYN:0.038".,G:Epsilon Ind group.
HR 5665			BD+23 2789	135263	83723	3201					15 13 31.9	+22 59 00	6.30	A2V
HR 5675		3	BD+05 2985	135482	120916	562	I				15 15 11.4	+04 56 22	5.33	K0III
HR 5679		4	BD+00 3327	135559	120920						15 15 49.1	+00 22 20	5.63	A4V
HR 5690			BD+00 3337	136028	140444		I				15 18 26.2	-00 27 41	5.89	K5III
HR 5692			BD+21 2755	136138	83755	1400					15 18 24.5	+20 34 22	5.70	G8IIIaBa0.3
HR 5694		5	BD+02 2944	136202	120946				9584	MQ Ser	15 19 18.8	+01 45 55	5.06	F8III-IV	4.6	11.2	D:AB binary. Some disagreement as to whether B or C, at 127" from A, is the brighter.,DYN:0.034".,G:Not member of Gamma Leo group but previously listed as such.
HR 5706			BD-01 3047	136442	140473						15 20 47.1	-02 24 48	6.35	K0V
HR 5710		6	BD+01 3067	136514	120955		I		9596	7037	15 21 02.0	+00 42 55	5.35	K3III	4.0	3.1	D:CPM?,DYN:0.013".,G:Wolf 630 group.
HR 5711			BD+25 2902	136643	83778						15 21 06.9	+24 57 28	6.39	K0
HR 5717		7	BD+13 2928	136831	101508	3213					15 22 23.2	+12 34 03	6.28	A0V
HR 5721		8	BD-00 2961	137006	140502	1406					15 23 43.7	-01 01 21	6.12	F0V			G:UMa stream.
HR 5739	τ¹	9	BD+15 2858	137471	101545	570	I			7074	15 25 47.4	+15 25 41	5.17	M1III
HR 5740			BD+19 2966	137510	101548						15 25 53.3	+19 28 51	6.27	G0IV-V			M:Possible nearby star on basis of spectroscopic parallax.
HR 5745			BD+25 2916	137853	83830	3219	I				15 27 38.9	+25 06 06	6.02	gM1
HR 5746		10	BD+02 2965	137898	121020	3221					15 28 38.2	+01 50 32	5.17	A8IV
HR 5758			BD+09 3055	138290	121038	1408					15 30 55.4	+08 34 45	6.57	F4V w
HR 5770	τ²	12	BD+16 2797	138527	101600						15 32 09.7	+16 03 22	6.22	B9V
HR 5772		11	BD-00 2982	138562	140596	3226					15 32 57.9	-01 11 11	5.51	K0III
HR 5783			BD+17 2880	138803	101618						15 33 52.8	+17 08 16	6.45 R	F3III
HR 5788	δ	13	BD+11 2821	138917	101623				9701 B		15 34 48.1	+10 32 15	3.80	F0IV	1.1	3.9	D:ADS 9701, 3168y, a = 5.8432". Binary with HR 5789, blended mag., colors.,DYN:0.022".
HR 5789	δ	13	BD+11 2821	138918	101624				9701 A	Del Ser	15 34 48.1	+10 32 21	3.80	F0IV	1.1	3.9	D:Binary with HR 5788. CD 13.5, 14.0 sep. 4" at 65" from A, optical.,DYN:0.022".,VAR:Delta Sct 4.20 - 4.25V, 0.134d. Fourier analysis of 1975 and 1979 data shows frequencies of 6.4227 and 7.8869 cycles/d,VAR:or periods 0.1557 and 0.1268d.
HR 5791			BD+02 2977	138936	121071						15 35 04.6	+01 40 08	6.56	F0III
HR 5795	τ³	15	BD+18 3044	139074	101631	3230					15 35 33.2	+17 39 20	6.12	gG8
HR 5796			BD+11 2826	139087	101634	3231					15 35 53.4	+11 15 56	6.07	gK0
HR 5799		14	BD-00 2988	139137	140643						15 36 33.7	-00 33 42	6.51	G8III+A
HR 5802		16	BD+10 2884	139195	101640						15 36 29.6	+10 00 36	5.26	K0III:CN1Ba0.7Sr2
HR 5804	τ⁵	18	BD+16 2807	139225	101642						15 36 29.3	+16 07 08	5.93	F3V			S:Also classified F0IVn.
HR 5831			BD+12 2875	139862	101673				9740		15 40 10.4	+12 03 11	6.25	G7.5IIIaFe-0.5	4.2	16.5	D:Companion 10.33V, +0.49(B-V), -0.01(U-B), F5V, CPM.,S:G8.5IIIa CN-1 Ca-1 Fe 0.5.
HR 5840	τ⁶	19	BD+16 2816	140027	101678						15 40 59.2	+16 01 29	6.01	G8III			G:Sirius group; UMa stream.
HR 5842	ι	21	BD+20 3138	140159	101682				9744		15 41 33.1	+19 40 13	4.52	A1V	0.1	0.1	D:AB 5.2 A1V, 5.3 AIV, 11.07y, a = 0.117". AB combined mag., color. Resolved by speckle interferometry 1986.45,,D:sep. 0.05".,DYN:0.012" to 0.026".,G:Pleiades group.
HR 5843	χ	20	BD+13 2982	140160	101683	3243				Chi Ser	15 41 47.4	+12 50 51	5.33	A0pSr v			G:In Ursa cluster; UMa stream. Possible Eggen group with HR 63, q.v.,VAR:Alpha CV 5.33 - 5.36V, 1.59584d. SrII same period. Magnetic field var. Period probably due to rotation of star,VAR:spots.
HR 5845	τ⁷	22	BD+18 3059	140232	101686						15 41 54.7	+18 27 50	5.81	A2m			G:Hyades group.,S:Also classified A8Vams.
HR 5850			BD+14 2922	140438	101699				9758		15 43 10.6	+13 40 04	6.48	G5III	1.0	0.6
HR 5853	ψ	23	BD+02 2989	140538	121152	3248			9763		15 44 01.8	+02 30 54	5.88	G2.5V	1.3	370.	D:Quintuple system of which E is brightest companion; B, 12.0V at 4"; others at 172" and 208".,DYN:0.084".
HR 5854	α	24	BD+06 3088	140573	121157	582	I		9765		15 44 16.1	+06 25 32	2.65	K2IIIbCN1	8.3	58.2	D:SR? Amp. 0.2V. ADS 9765B, optical.,N:UNUKALHAI; Unuk al Hay; Unuk Elhaia; Unuk; Unukalhay; Cor Serpentis.
HR 5858	τ⁸	26	BD+17 2906	140729	101712			S			15 44 42.1	+17 15 51	6.14	A0V		0.1
HR 5859			BD+05 3072	140775	121170						15 45 23.5	+05 26 49	5.58	A0V			G:UMa stream.
HR 5861			BD+01 3125	140815	121173						15 45 39.7	+00 53 29	6.33	K0III
HR 5863		25	BD-01 3092	140873	140740						15 46 05.6	-01 48 16	5.40	B8III			SB:38.937d, K 53.6k/s, V0 -12.6k/s, asini 17.2. Unresolved by speckle interferometry.
HR 5867	β	28	BD+15 2911	141003	101725	583			9778		15 46 11.3	+15 25 19	3.67	A2IV	6.3	30.6	D:B, 9.72V, +0.84(B-V), +0.68(U-B), K3V, CPM. C, 10.7v at 201". Also CPM with BD+15d2906 at 1642", itself a double, 8.4,,D:10.5v sep. 6".,DYN:0.016".,G:Sirius group; member of Ursa cluster; UMa stream.,RV:ADS 9778B, +2.8k/s.
HR 5868	λ	27	BD+07 3023	141004	121186		I			7246	15 46 26.6	+07 21 11	4.43	G0-V			SB:1837d, K 2.8k/s, V0 -6.7k/s, asini 59.1. Orbit questioned by Morbey and Griffin (1987, ApJ, 317, 343).
HR 5870	υ	31	BD+14 2939	141187	101739						15 47 17.3	+14 06 55	5.71	A3V			G:Hyades group.
HR 5874			BD+14 2940	141353	101744		I				15 48 13.3	+13 47 19	6.00	gK2
HR 5879	κ	35	BD+18 3074	141477	101752	584	I			7269	15 48 44.4	+18 08 30	4.09	M0.5IIIab e			S:Ultraviolet FeII emission.
HR 5881	μ	32	BD-02 4052	141513	140787	585					15 49 37.2	-03 25 49	3.53	A0V
HR 5888	ω	34	BD+02 3007	141680	121215		I				15 50 17.5	+02 11 47	5.23	G8III			G:UMa stream.,S:Also classified A6IVm.
HR 5892	ε	37	BD+04 3069	141795	121218	588					15 50 49.0	+04 28 40	3.71	A2Vm			S:Also classified A6IVm.
HR 5894			BD+15 2918	141850	101771		I			R Ser	15 50 41.7	+15 08 01	5.20	M7IIIe			VAR:M 5.16 - 14.4v, 356.41d.
HR 5895		36	BD-02 4058	141851	140801			S			15 51 15.6	-03 05 26	5.11	A3Vnp		0.1	S:Lambda Boo star, Mg 4481 wk.
HR 5899	ρ	38	BD+21 2829	141992	84037		I			7300	15 51 15.9	+20 58 40	4.76	K5-III
HR 5909			BD+17 2926	142244	101789						15 52 56.2	+17 24 13	6.36 R	K0
HR 5911		39	BD+13 3024	142267	101792	3254		W		7313	15 53 12.1	+13 11 48	6.10	G0VFe-0.5	5.6	98.3
HR 5913			BD+16 2840	142357	101796				9828		15 53 34.9	+16 04 30	6.09 R	F5II-III	6.4	3.6	S:Also classified F4IVs or F3V.
HR 5919		40	BD+09 3116	142500	121254	3256				FP Ser	15 54 40.3	+08 34 49	6.29	A7Vn			VAR:Delta Sct 6.20 - 6.23V, about 0.250d.
HR 5924			BD+20 3166	142574	84070	3257	I				15 54 34.6	+20 18 39	5.44	M0III			G:Epsilon Ind group.,M:High space velocity.
HR 5931			BD+19 3036	142763	101821						15 55 39.8	+18 37 14	6.26	B8III			M:Old disk population runaway star.
HR 5933	γ	41	BD+16 2849	142860	101826	591	I	W		7350	15 56 27.2	+15 39 42	3.85	F6V	6.6	201.5	C:Color excess E(B-V) = +0.03.,D:Companions optical?
HR 5940	φ		BD+14 2969	142980	101834		I				15 57 14.6	+14 24 52	5.54	K1IV
HR 5963			BD+04 3096	143553	121315	3262					16 00 51.1	+04 25 39	5.83	gK0
HR 5972	π	44	BD+23 2886	143894	84155	3268					16 02 17.7	+22 48 16	4.83	A3V
HR 5976		43	BD+05 3131	144046	121339			W			16 03 45.7	+04 59 12	6.08	G9III	7.8	30.8	G:Probable Hyades group.
HR 5992			BD+08 3134	144426	121361						16 05 37.8	+08 05 46	6.29	A3m			SB:8.855d, K 31.6k/s, V0 -21.5k/s, asini 3.56.
HR 6004		45	BD+10 2958	144874	101939	3274					16 07 37.5	+09 53 30	5.63	A7V
HR 6005			BD+22 2926	144889	84202		I				16 07 22.2	+21 49 21	6.14	K4III
HR 6010		47	BD+08 3141	145002	121383		I			FS Ser	16 08 28.0	+08 32 03	5.73	M3.5IIIa			VAR:Amp. 0.04V.
HR 6011			BD+03 3132	145085	121390		I				16 08 58.9	+03 27 16	5.91	gK5
HR 6014			BD+06 3169	145148	121392	1422					16 09 11.2	+06 22 44	5.97	K1.5IV
HR 6016			BD-03 3884	145206	141001		I				16 09 50.5	-03 28 01	5.37	K4III			SB:Companion may be the cause of bright UV in spectrum.
HR 6093	σ	50	BD+01 3215	147449	121540	1427					16 22 04.4	+01 01 45	4.82	F0V			G:Hyades group.
HR 6446	ν	53	BD-12 4722	156928	160479	3376			10481		17 20 49.7	-12 50 49	4.33	A2V	4.8	46.3	G:Possible Eggen group with HR 63, q.v.
HR 6449			BD-10 4477	156971	160482			W			17 20 52.7	-10 41 46	6.46	F1III	7.8	8.1
HR 6496			BD-12 4750	157968	160553						17 27 02.1	-12 30 45	6.21	F7V			N:Originally called 47 Oph; now in Serpens.
HR 6544			BD-11 4411	159358	160653	1461		W			17 34 46.4	-11 14 31	5.55	B8Vn	3.0	54.6	G:Sco-Cen assoc.
HR 6561	ξ	55	BD-15 4621	159876	160700	658	I	W		9270	17 37 35.2	-15 23 55	3.54	F0IVDel Sct	9.4	22.0	D:Visual companion optical.,G:Hyades moving group.,SB:2.2923d, K 19.4k/s, V0 -42.8k/s, asini 0.612.,VAR:Delta Sct?, 3.52 - 3.54V.
HR 6562			BD-15 4622	159877	160701						17 37 36.2	-15 34 16	5.94	F0IV
HR 6568			BD-10 4528	160018	160708		I				17 38 09.5	-10 55 35	5.75	gK0
HR 6581	ο	56	BD-12 4808	160613	160747	3405				Omi Ser	17 41 24.9	-12 52 31	4.26	A2V			VAR:Delta Sct 4.20 - 4.26V, 0.053d.
HR 6600			BD-13 4732	161023	160784						17 43 48.6	-13 30 31	6.39	F0V
HR 6620			BD-14 4770	161701	160822	3413					17 47 36.8	-14 43 33	5.94	B9pHgMn			G:Member of Pleiades group.,SB:12.4520d, K 52.5k/s, V0 -18.5k/s, asini 8.97.
HR 6666			BD-10 4560	162757	160885						17 53 03.6	-10 53 59	6.18	gK1
HR 6681			BD-15 4722	163336	160915				10891		17 56 19.0	-15 48 45	5.89	A1V	3.2	20.6	D:AB CPM; C, 12v at 34" optical.
HR 6710	ζ	57	BD-03 4217	164259	142025						18 00 29.0	-03 41 25	4.62	F2IV
HR 6755			BD-08 4558	165402	142083	3436					18 06 07.4	-08 19 26	5.85	B8III-IV			G:Sco-Cen assoc.
HR 6756			BD-04 4395	165438	142085						18 06 15.2	-04 45 05	5.77	K1+IV
HR 6785			BD-13 4863	166103	161125	1472	I				18 09 43.4	-13 56 04	6.39	K0
HR 6813			BD-04 4415	166960	142159	3450					18 13 10.0	-04 00 42	6.59	A2m
HR 6830			BD-03 4259	167564	142185						18 15 58.0	-03 37 03	6.36	A4V
HR 6840			BD-03 4263	167768	142189						18 16 53.1	-03 00 26	6.00	G3III			G:Arcturus group?
HR 6843			BD-09 4678	167833	142192	1475					18 17 24.2	-09 45 31	6.31	A8V
HR 6858			BD-15 4927	168415	161348		I				18 20 08.8	-15 49 54	5.39	K4III
HR 6869	η	58	BD-02 4599	168723	142241	688	I	W		10675	18 21 18.6	-02 53 56	3.26	K0III-IV	8.7	179.7	S:Also classified K0III-IV.
HR 6873			BD+05 3704	168797	123385					10688	18 21 28.5	+05 26 09	6.13	B3Ve			S:Shell star.,VAR:6.11 - 6.14V. Emission variable 12 to over 22 yrs.
HR 6890			BD-03 4277	169268	142274						18 24 03.5	-03 35 00	6.38	F6III-IV			SB:Equal components.
HR 6898			BD-01 3486	169493	142294				11324		18 24 57.0	-01 34 46	6.15	F6III+A9III	0.4	0.8	D:6.8 F6III, 7.0 A7IV, 240y, a = 0.59". Combined mag., colors.
HR 6900			BD+05 3730	169578	123453						18 25 08.8	+05 05 05	6.74	B9V
HR 6918		59	BD+00 3936	169985	123497				11353	d Ser	18 27 12.5	+00 11 46	5.21	G0III+A6V	2.3	3.8	D:AB physical. B is F5V, vsini =<54k/s. Component P, vsini 80:k/s.,DYN:0.007".,SB:ADS 11353A is triple spectroscopic system with periods 385 and 1.8505205d. vsini of A-type component 270k/s, of G-type,,SB:80:k/s. Comp. B may also be SB, and third visual component P at 0.1" from A may be one of the components of the long,SB:period pair. ADS 11353A, 1.8505, K 90k/s, asini 2.29. ADS 11353Ap?, 386.0d, K 28k/s, V0 -23.3k/s, asini 731.,SB:Companion with sep. 0.25" seen only on 1976.61; unresolved at four other epochs between 1976.3 and 1979.5 (McAlister,SB:and Hartkopf).,SB:28k/s, V0 -23.3k/s, asini 731.,VAR:ADS 11353A, 4.9 - 5.9v.
HR 6928			BD+06 3790	170200	123516			S			18 27 58.8	+06 11 39	5.73	B8III-IV		0.1	G:Hyades group; NGC 6633 #102.,SB:3.4941d, K 38.5k/s, V0 -14.7k/s, asini 1.85. Mass loss from primary. If mass ejection discontinuous, mag. may,SB:remain constant over long intervals.
HR 6935		60	BD-02 4641	170474	142348	1480					18 29 41.0	-01 59 07	5.39	K0III			SB:3.1558d, K 3.6k/s.
HR 6957		61	BD-01 3504	170920	142372						18 31 57.0	-01 00 11	5.94	A4III			N:Some older catalogues following BAC call this e Ser. However, Heis and followers, including HR, call HR 6993 = e.
HR 6958			BD+03 3737	170973	123610					MV Ser	18 32 07.0	+03 39 35	6.43	A0pSiCr			S:Magnetic star. Also classified B9.5IVp.,VAR:0.945099d, amp. 0.03U.
HR 6993			BD-00 3521	171978	142444	3480				11122	18 37 36.0	-00 18 34	5.75	A1V+A1V			G:Sirius group? UMa stream; UMa cluster.,SB:14.674d, K 38.6k/s, V0 +11.4k/s, msin3i 0.319, asini 7.62, i 29d, vsini 26 and <26k/s.
HR 6999			BD-03 4331	172088	142461				11520		18 38 23.7	-03 11 37	6.49	F9IV	0.1	0.1	D:AB 7.2 F9V, 7.3 F9V, sep. 0.13", 12.18y, a = 0.196". Measured sep. 0.141" on 1985.5 by speckle interferometry. Third,D:component 14v, optical.,DYN:0.028".
HR 7000			BD-01 3529	172103	142460						18 38 19.1	-01 06 48	6.66	F1IV-V
HR 7008			BD+05 3891	172365	123778	3485					18 39 36.9	+05 15 51	6.38	F8Ib-II			G:IC 4756 #145.,S:CNO content high relative to (Fe/H) and Lithium abundance high (at or near interstellar value).
HR 7048			BD+05 3941	173495	123886				11640		18 45 28.4	+05 29 59	5.83	A1V+A1V	0.3	1.3	D:ADS 11640AB, >5600y. Both components close binaries. Speckle interferometry 1985.5 gives sep. Aa = 0.141";,D:Bb = 0.137".,SB:ADS 11640A. A1, A4.
HR 7076			BD+04 3884	173954	123928	3494	I				18 48 02.7	+04 14 29	6.21	K5 v			S:Profiles of H alpha and H beta emission vary.
HR 7141	θ¹	63	BD+04 3916	175638	124068	709			11853 A	11557	18 56 13.2	+04 12 13	4.62	A5V	0.4	22.2	D:Binary with HR 7142.,DYN:0.019".,G:Hyades group.,N:Alya; Alga.,VAR:4.59 - 4.72V.
HR 7142	θ²	63	BD+04 3917	175639	124070				11853 B		18 56 14.6	+04 12 07	4.98	A5Vn	0.4	22.2	D:Binary with HR 7141.,DYN:0.019".
HR 7144			BD+02 3730	175679	124073			W			18 56 25.6	+02 28 16	6.15	G8III	5.7	100.
HR 7158		64	BD+02 3738	175869	124089						18 57 16.6	+02 32 07	5.57	B9IIIep:Hg: v			G:Member of the local association (Pleiades group).,S:H alpha emission.,VAR:Hydrogen line widths vary in cycles of about 10 yrs.

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

Serpens / Yale Bright Star Catalog (HR)

Legende

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