Kataloge

Katalog

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Hercules / 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 5914	χ	1	BD+42 2648	142373	45772	1416					15 52 40.5	+42 27 06	4.62	F8VFe-2Hdel -1			S:Lithium to hydrogen ratio about 12 times solar. Low metal content.,VAR:Variable intrinsic polarization observed Aug. 1974.
HR 5932		2	BD+43 2542	142780	45788		I			7335	15 54 37.9	+43 08 19	5.37	M3IIIBa0.3
HR 5938		4	BD+42 2652	142926	45790					Var?	15 55 30.6	+42 33 58	5.75	B9pe v			S:Shell star. Also classified B8V.,SB:46.0227d, K 12.0k/s, V0 -19.3k/s, asini 7.17. RV period constant over 40 yrs. Shell-line RV also 46.023d.,VAR:Spectrum var. Balmer emission and metallic absorption vary in period about 30 yrs; H alpha profile varies in period,VAR:of =<1 min. A potassium flare observed June 21, 1965. Probable mass-transfer between components.
HR 5950			BD+40 2948	143209	64988						15 57 29.9	+39 41 43	6.31	K0			G:Probable Hyades group.
HR 5964			BD+50 2239	143584	29737	3260					15 59 04.4	+49 52 52	6.05	F0IV
HR 5966		5	BD+18 3101	143666	101879	3263	I				16 01 14.3	+17 49 06	5.12	G8IIIbFe-0.5
HR 5982	υ	6	BD+46 2142	144206	45865	3271					16 02 47.9	+46 02 12	4.76	B9III			S:HgMn star.
HR 6008	κ	7	BD+17 2964	145001	101951	1421			9933 A	7471	16 08 04.5	+17 02 49	5.00	G8III	1.2	28.1	D:Optical pair with HR 6009.,N:Marfik; Marsik; Mirfak; Marfak.,S:Also classified G8II, G7III.
HR 6009	κ	7	BD+17 2965	145000	101952		I		9938 B		16 08 04.9	+17 03 16	6.25	K1III	1.2	28.1	D:Optical pair with HR 6008.,S:Also classified K0IV, K2II and K2III.
HR 6013		8	BD+17 2967	145122	101962					7477	16 08 46.6	+17 12 21	6.14	A0Vnn
HR 6023	φ	11	BD+45 2376	145389	45911	601				7490	16 08 46.2	+44 56 06	4.26	B9p:Mn:			S:HgMn star.,SB:560.5d, K 2.4k/s, V0 -16.8k/s, asini 16.3. Unresolved by speckle interferometry 1986.45.,VAR:Alpha CV?, 4.23 - 4.27V, amp. 0.015U, 7.832d, symmetric light curve.
HR 6032			BD+10 2971	145589	121414			W			16 11 29.7	+09 42 45	6.53	F0IV	0.0	0.1	D:A5, F1.
HR 6035			BD+17 2982	145647	101994	3279					16 11 28.7	+16 39 56	6.08	A0V
HR 6039		10	BD+23 2909	145713	84240		I			LQ Her	16 11 38.0	+23 29 41	5.70	M4.5IIIa			VAR:Lb? 5.58 - 5.83V, 7.1 - 7.31p.
HR 6047		9	BD+05 3165	145892	121431	3283	I				16 13 15.4	+05 01 16	5.48	gK5
HR 6050			BD+42 2683	145931	45957	3281	I		9962		16 11 47.6	+42 22 28	5.87	K4II+F6-8V	4.3	23.6	D:Companion, 10.73V, +0.58(B-V), +0.08(U-V), F8IV:, CPM.
HR 6057			BD+06 3184	146084	121443						16 14 13.5	+05 54 07	6.31	K2III
HR 6065		16	BD+19 3075	146388	102040						16 15 28.7	+18 48 30	5.69	K3III
HR 6087			BD+21 2902	147266	84306						16 20 04.3	+21 07 57	6.05	G8IIIb
HR 6090			BD+49 2491	147352	46025	3292	I				16 19 11.2	+49 02 17	5.91	gK6
HR 6091			BD+40 3005	147365	65233	3293		W			16 19 55.1	+39 42 31	5.46	F3IV-V	4.5	2.2	D:CPM.
HR 6092	τ	22	BD+46 2169	147394	46028	608			10010	7641	16 19 44.4	+46 18 48	3.89	B5IV	10.7	6.7	D:ADS 10010AB, 6700y.,VAR:3.85 - 3.90V.
HR 6095	γ	20	BD+19 3086	147547	102107	609	I		10022	7667	16 21 55.2	+19 09 11	3.75	A9III	6.4	41.6	D:ADS 10022B, 9.58v, optical.,G:Hyades group.,SB:11.9d.
HR 6111		21	BD+07 3164	147869	121568	1429					16 24 10.8	+06 56 53	5.85	A2pSr:			SB:4.951d, K 16.3k/s, V0 -34.4k/s, asini 0.955.
HR 6117	ω	24	BD+14 3049	148112	102153	613			10054	Ome Her	16 25 25.0	+14 02 00	4.57	B9pCr	8.1	28.4	D:B, 12.0v at 2" CPM; C optical.,G:UMa stream; Sirius group.,N:Kajam; Cujam; Cajam; Caiam.,S:Also classified A2VpCrMnSr.,VAR:Alpha CV, amp. 0.08V, 2.951d, double wave light curve. Also rapid var. 0.15d.
HR 6119			BD+19 3098	148206	102160		I			U Her	16 25 47.7	+18 53 33	6.70	M7IIIe			S:SiO maser emission. Infrared star showing OH and H2O emission.,VAR:ADS 10449A, M 6.5 - 13.3v, 406.05d.
HR 6121			BD+11 2984	148228	102165						16 26 11.5	+11 24 27	6.11	G8III
HR 6123		25	BD+37 2750	148283	65290	3296		S			16 25 24.2	+37 23 38	5.54	A5V		0.2	S:Shell star.
HR 6146		30	BD+42 2714	148783	46108	3303	I			g Her	16 28 38.5	+41 52 54	5.04	M6-III			VAR:SRb 4.3 - 6.3v, 5.7 - 7.2p, 89.2d. Also slow var. of about 875d and aperiodic superposed cycles 5 - 15d.
HR 6148	β	27	BD+21 2934	148856	84411	618	I	W		7778	16 30 13.2	+21 29 23	2.77	G7IIIa	7.3	256.2	D:Visual companion probably optical.,N:Kornephoros; Korneforos; Rutilicus.,SB:410.575d, K 12.8k/s, V0 -25.5k/s, asini 60.4. Unresolved by speckle interferometry.
HR 6152			BD+20 3283	148897	84416		I			7785	16 30 33.6	+20 28 45	5.25	G8IIICN-2CH-1			G:Wolf 630 group.,S:Also classified G8IIICN-2CH-0.5Ca0.5.
HR 6154			BD+22 2983	149009	84423		I				16 31 13.4	+22 11 43	5.76	gK5
HR 6156		34	BD+49 2514	149081	46128						16 30 06.0	+48 57 39	6.45	A1V
HR 6157			BD+35 2828	149084	65356	3308	I				16 31 02.8	+35 13 30	6.25	K5
HR 6158		28	BD+05 3223	149121	121676	3309					16 32 35.7	+05 31 16	5.63	B9.5III
HR 6159		29	BD+11 3008	149161	102234	3310	I			7812	16 32 36.3	+11 29 17	4.84	K7III			VAR:4.82 - 4.85V.
HR 6162			BD+45 2422	149303	46147				10105		16 31 47.3	+45 35 54	5.65	A4Vn	3.3	16.3
HR 6168	σ	35	BD+42 2724	149630	46161	621		S		7837	16 34 06.2	+42 26 13	4.20	B9V	3.	0.1	D:Sep. 0.067". Noted as double by speckle interferometry in 1971-2, unresolved at Mayall 4-meter in 1976. Spectrum,D:double-lined. Resolved by speckle observations 1986.45 (Blazit et al. 1987, A&AS, 71, 57).
HR 6169			BD+17 3053	149632	102259	3313		W			16 35 26.3	+17 03 26	6.41	A2V	1.0	156.6	D:Companion A2V, CPM; vsini 80k/s.,SB:10.56d, K 62.4k/s, V0 -9.9k/s, msin3i 2.20, asini 8.18.
HR 6176			BD+15 3029	149822	102271					V773 Her	16 36 43.0	+15 29 53	6.30	B9pSiCrSr:			G:Wolf 630 group.,VAR:Alpha CV, amp. 0.03U, 0.02B, 0.01V, 1.45876d.
HR 6181			BD+13 3177	150012	102278	3316					16 37 48.0	+13 41 13	6.31	F5IV			S:Also classified F4V.
HR 6183			BD+46 2194	150030	46184	3314					16 36 11.2	+46 36 48	5.79	G8II
HR 6194		36	BD+04 3234	150379	121774				10149 B		16 40 35.1	+04 12 26	6.93	A3IV	1.2	69.6	D:Binary with HR 6195. Component B is speckle binary, sep. 0.145". Component C, optical. A companion 0.145" from B,D:discovered by speckle interferometry.
HR 6195		37	BD+04 3235	150378	121776				10149 A		16 40 38.7	+04 13 11	5.77	A1V	1.2	69.6	D:Binary with HR 6194, q.v.
HR 6200		42	BD+49 2531	150450	46210	1434	I		10144	7896	16 38 44.9	+48 55 42	4.90	M2.5IIIab	5.4	25.6	D:Optical.
HR 6203			BD+12 3063	150483	102314						16 40 51.4	+12 23 42	6.08	A3Vn
HR 6208			BD+25 3115	150580	84536	3323	I				16 41 00.6	+24 51 31	6.06	K2
HR 6212	ζ	40	BD+31 2884	150680	65485		I		10157	7915	16 41 17.2	+31 36 11	2.81	G0IV	2.6	1.1	D:ADS 10157AB, 2.90 F9IV, 5.53 G7V, 34.49y, a = 1.355". ADS 10157A*, 10.5y, a = 0.08".,DYN:0.096".,G:Zeta Her group.,SB:ADS 10157A, 34.417y D, K 3.8k/s, V0 -69.9k/s, asini 590. Resolved by speckle interferometry.,VAR:ADS 10157A is var. suspect NSV 7915.
HR 6213		39	BD+27 2668	150682	84543			S			16 41 36.7	+26 55 01	5.92	F2III		0.1	SB:2.3076d, K 100.6k/s, V0 -9.0k/s, msin3i 1.14, asini 3.19.
HR 6220	η	44	BD+39 3029	150997	65504	626	I	W		7934	16 42 53.8	+38 55 20	3.53	G7.5IIIbFe-1		113.5	D:Companion questioned.
HR 6222			BD+34 2830	151087	65512	3330					16 43 51.7	+34 02 20	5.99	F2-3III-IV
HR 6227			BD+16 3013	151203	102365		I			7950	16 45 22.5	+15 44 43	5.56	M3IIIab
HR 6228		43	BD+08 3271	151217	121843	3332	I	W		7952	16 45 49.9	+08 34 57	5.15	K5III	3.9	82.5
HR 6230			BD+43 2642	151388	46262		I				16 45 11.7	+43 13 02	6.05	K4III
HR 6234		45	BD+05 3272	151525	121865	3333		W		V776 Her	16 47 46.4	+05 14 48	5.24	B9pCr:	5.2	122.7	G:Possible Pleiades group.,S:Oxygen deficient relative to magnesium.,VAR:Alpha CV, 5.21 - 5.27V, amp. 0.04U, 1.31159d.
HR 6239			BD+13 3225	151627	102393						16 48 08.9	+13 35 26	6.35	G5III
HR 6242			BD+42 2749	151732	46288	3336	I			V636 Her	16 47 19.8	+42 14 20	5.87	M4+III-IIIa			VAR:Lb 5.83 - 6.03V.
HR 6246			BD+13 3233	151862	102410				10225		16 49 34.6	+13 15 41	5.91	A1V	4.0	5.3
HR 6250		47	BD+07 3256	151956	121895					7990	16 50 19.4	+07 14 52	5.49	A3m			G:Possible Eggen group with HR 63, q.v.,VAR:5.5 - 5.54V.
HR 6254		52	BD+46 2220	152107	46305				10227	V637 Her	16 49 14.2	+45 59 00	4.82	A2VpSrCrEu v	4.6	1.8	D:BC 9.0, 9.1, 56.75y, a = 0.267". AxBC physical.,DYN:0.024".,G:Sirius group. UMa stream.,S:Oxygen deficient relative to magnesium. Magnetic star, also classified A3VpSrCrEuMn.,VAR:ADS 10227A, Alpha CV 4.78 - 4.83V, 3.8567d. K line varies, 3.88d.
HR 6256			BD+43 2654	152153	46311						16 49 40.5	+43 25 50	6.13	K0IV
HR 6258		50	BD+30 2884	152173	84641	3339	I				16 50 39.0	+29 48 24	5.72	M1IIIa
HR 6259			BD+32 2795	152224	65595						16 50 43.1	+32 33 13	6.13	K0III
HR 6264			BD+42 2753	152262	46317						16 50 36.1	+41 53 48	6.29	gK3
HR 6268		49	BD+15 3066	152308	102435	629				V823 Her	16 52 04.9	+14 58 27	6.52	B9.5pCr:
HR 6270		51	BD+24 3069	152326	84651	1440	I				16 51 45.3	+24 39 23	5.04	K0.5IIIaCa0.5
HR 6279		53	BD+31 2925	152598	65627	1441		W			16 52 58.1	+31 42 06	5.32	F0-2V	6.7	70.9
HR 6286			BD+47 2400	152812	46349		I	S			16 53 17.6	+47 25 01	6.00	K2III		0.3
HR 6287			BD+21 3002	152815	84687	3343					16 54 55.2	+20 57 31	5.41	G8III
HR 6290			BD+13 3258	152830	102474					V644 Her	16 55 16.0	+13 37 11	6.34	F3V s			S:Previously classified F5II, unusual luminosity for Delta Sct type var.,SB:11.848d, K 28.5k/s, V0 -3.7k/s, asini 4.41.,VAR:Delta Sct 6.32 - 6.36V, 0.11505449d.
HR 6292		56	BD+25 3156	152863	84692				10259		16 55 02.1	+25 43 50	6.08	G5III	4.6	17.9	D:CPM.,G:Sirius group? UMa stream.
HR 6293		54	BD+18 3266	152879	102476		I		10262		16 55 22.2	+18 26 00	5.35	K4III	4.2	2.5	D:AC, CPM. C, 12.5v at 93".
HR 6301			BD+14 3155	153226	102496	3346					16 57 32.0	+13 53 03	6.37	K0V			M:Possible nearby star on basis of spectroscopic parallax.
HR 6305		57	BD+25 3166	153287	84720						16 57 31.0	+25 21 10	6.28	gG5
HR 6306			BD+50 2345	153299	30161		I				16 56 06.4	+50 02 20	6.56	M2IIIab
HR 6307			BD+24 3095	153312	84726	3347					16 57 42.3	+24 22 53	6.32	K0III
HR 6313			BD+42 2774	153472	46401	3349					16 57 50.2	+42 30 45	6.34	K3III
HR 6324	ε	58	BD+31 2947	153808	65716	634					17 00 17.4	+30 55 35	3.92	A0V			SB:4.0235d, K 70.7k/s, V0 -24.2k/s, msin3i 1.56, asini 3.91.
HR 6325			BD+22 3045	153834	84758		I				17 00 58.1	+22 37 56	5.65	gK3
HR 6326			BD+15 3095	153882	102536				10310	V451 Her	17 01 33.0	+14 56 58	6.31	B9pCrEu v	4.6	19.0	D:Fixed sep.,VAR:ADS 10310A, Alpha CV 6.26 - 6.34V, 6.00925d. Spectrum, magnetic field, RV, same period. Rotation 6.0087d.
HR 6328			BD+27 2738	153897	84765						17 01 09.6	+27 11 47	6.55	F5V
HR 6332		59	BD+33 2817	154029	65736	1446					17 01 36.4	+33 34 06	5.25	A3IV
HR 6333			BD+25 3183	154084	84776	3356					17 02 18.7	+25 30 20	5.75	gG7
HR 6336			BD+32 2835	154126	65745						17 02 17.2	+31 53 05	6.36	K0
HR 6337			BD+14 3179	154143	102553		I			8142	17 03 07.8	+14 05 31	4.98	M3III			G:Gamma Leo group.
HR 6339			BD+14 3180	154160	102554					8143	17 03 10.4	+14 30 40	6.52	G5IV:
HR 6341			BD+13 3292	154228	102564			W		8152	17 03 39.3	+13 36 19	5.93	A1V	0.2	299.2
HR 6342			BD+13 3295	154278	102569						17 03 58.0	+13 34 03	6.08	K1III			D:Component B of system with HR 6341.,G:Gamma Leo group.
HR 6343			BD+19 3218	154301	102571		I		10323	8158	17 03 52.7	+19 41 26	6.35	K4III	4.3	108.1	D:B, 11.0v at 1.5" CPM.,VAR:ADS 10323B, 10 - 11.3v?
HR 6346		61	BD+35 2911	154356	65761		I			8159	17 03 30.2	+35 24 51	6.69 R	M4IIIab
HR 6351			BD+34 2890	154431	65766						17 03 53.5	+34 47 25	6.04 R	A5V
HR 6352			BD+19 3220	154441	102579				10326		17 04 41.3	+19 35 57	6.17 R	B9.5V	3.0	1.9
HR 6355		60	BD+12 3142	154494	102584	635			10334		17 05 22.7	+12 44 27	4.91	A4IV	6.1	56.0	D:Optical.,G:Possible Eggen group with HR 63, q.v.
HR 6362			BD+44 2652	154713	46478	1448					17 05 05.0	+43 48 44	6.43	A3IV
HR 6363			BD+49 2583	154732	46476	3359				8185	17 04 49.8	+48 48 15	6.09	K1III			G:Gamma Leo group.,SB:786d, K 10.0k/s, V0 +12.8k/s, asini 103.,VAR:6.7 - 6.9p.
HR 6364			BD+22 3073	154733	84835	3360	I		10343		17 06 18.1	+22 05 03	5.56	K3III	7.9	30.3	D:Optical.
HR 6376			BD+40 3103	155102	46502	636					17 07 46.7	+40 30 58	6.34	A2IV
HR 6377			BD+36 2827	155103	65812				10360		17 08 02.0	+35 56 07	5.39	A5-F1III/IVm s	0.1	0.1	D:AB 6.2 A9III-IV, 6.2 A9III-IV, 8.159y, a = 0.116". Mean mass 2.7 solar. Alternate orbit, 16.08y, a = 0.167". Combined,D:colors. Speckle interferometry indicates companion 1 mag. fainter than primary at 0.079". However, speckle,D:observations 1986.46 (at 7000 Ang.) give sep. 0.15".,DYN:0.017".,S:K/H/met give A5/F0V/F2.
HR 6388			BD+40 3109	155410	46524	3365	I	S			17 09 33.3	+40 46 38	5.08	K3III			SB:876.25d, K 4.79k/s, V0 -57.58k/s, asini 45.8. Unresolved at 10 epochs between 1977.69 and 1981.47 with sep. 0.039",SB:on 1980.48 (McAlister and Hartkopf).
HR 6391		63	BD+24 3140	155514	84896					V620 Her	17 11 03.2	+24 14 16	6.19	A8V			VAR:Delta Sct 6.19 - 6.23V. Period analyses of new and existing data by Reed and Welch (1988, AJ, 95, 1510) favor,VAR:fundamental period of 0.088d with overtones of 0.052, 0.130d, with the fundamental and second values as radial,VAR:pulsations and the third as nonradial.
HR 6399			BD+49 2604	155860	46561				10397	8327	17 11 40.2	+49 44 48	6.04 R	A5III	3.4	5.2	D:AB, CPM.
HR 6406	α¹	64	BD+14 3207	156014	102680		I		10418 A	Alp Her	17 14 38.9	+14 23 25	3.48 H	M5Ib-II e	2.2	4.9	D:AB, 3600y, a = 4.68". Component B is HR 6407. Combined colors. Combined mag. 3.08V. Mass A, 14 solar. Other components,D:faint, optical. Circumstellar lines around both A, B.,DYN:0.008".,N:RASALGETHI; Ras Algethi; Rasalegti.,R:Diam. = 0.020 - 0.030".,S:Ultraviolet FeII emission. 5-micrometer observations indicate carbon monoxide.,VAR:ADS 10418A. Discovered by W. Herschel in 1795. SRc 3.0 - 4.0v. 6-yr. period superimposed by variations 50 - 155d.,VAR:Surrounded by envelope of 2x10E+05 solar radii, expanding 10k/s, mass loss 3x10E-08 solar masses/y.
HR 6407	α²	64	BD+14 3207	156015	102681				10418 B		17 14 39.2	+14 23 24	5.39 H	G5III+F2V	2.2	4.9	C:IR source.,D:See HR 6406.,DYN:0.008".,SB:51.578d, K 36.1k/s, V0 -38.4k/s, asini 25.6. Sp. of fainter comp. of the SB, A3V, may be a collapsed star. Masses,SB:4.1, 2.5 Suns.
HR 6410	δ	65	BD+25 3221	156164	84951	641	I		10424	8419	17 15 01.9	+24 50 21	3.14	A3IV	5.6	8.5	D:ADS 10424B, dG4, optical.,N:Sarin.
HR 6418	π	67	BD+36 2844	156283	65890	643	I			8431	17 15 02.8	+36 48 33	3.16	K3IIab e			G:Red star Pleiades group.,S:Ultraviolet FeII emission.
HR 6419			BD+23 3070	156284	84955		I				17 15 41.6	+23 44 34	5.96	K2III
HR 6430			BD+23 3074	156593	84982		I				17 17 35.9	+23 05 27	6.45 R	K2
HR 6431		68	BD+33 2864	156633	65913				10449	u Her	17 17 19.5	+33 06 00	4.82	B1.5Vp+B5III	5.1	4.4	D:Binary.,DYN:0.010".,SB:ADS 10449A, B2.5V, B5V, 2.0510d, K 95.6k/s, V0 -30.0k/s, msin3i 7.16, asini 2.69. Semi-detached system. vsini of,SB:secondary 88k/s.,VAR:ADS 10449A, EA 4.69 - 5.37V, 2.0510270d. i 75.9d. Semi-detached system. Polarization measures indicate light from,VAR:primary reflected on photosphere of secondary.
HR 6432			BD+17 3216	156653	102724						17 18 05.0	+17 19 05	6.00	A1V
HR 6436		69	BD+37 2864	156729	65921					8489	17 17 40.3	+37 17 30	4.65	A2V
HR 6437			BD+49 2614	156753	46605						17 16 48.6	+49 41 28	7.48 R	K2
HR 6443			BD+28 2719	156874	85001	3375					17 18 48.5	+28 49 23	5.65	K0III
HR 6444			BD+38 2910	156891	65930	3373					17 18 23.3	+38 48 41	5.94	gG7
HR 6452			BD+18 3351	157049	102757	1454	I			V656 Her	17 20 18.9	+18 03 26	5.00	M2IIIab			VAR:Lb? 4.9 - 5.1v, amp. 0.16p.
HR 6455			BD+25 3246	157087	85016						17 20 09.8	+25 32 15	5.38	A3III
HR 6457		70	BD+24 3167	157198	85021			W			17 20 54.2	+24 29 58	5.12	A2V	3.5	222.9
HR 6458		72	BD+32 2896	157214	65963	1456			10488	8553	17 20 39.6	+32 28 04	5.39	G0V	5.1	230.0	D:B not CPM; optical.,VAR:Amp. 0.4V.
HR 6463			BD+16 3163	157257	102770		I				17 21 33.4	+16 43 51	6.35	M2.5IIIab
HR 6464		74	BD+46 2293	157325	46645	3377	I			8556	17 20 21.1	+46 14 27	5.59	M0III			G:61 Cyg group.
HR 6466			BD+28 2728	157358	85028			W			17 21 31.2	+28 45 29	6.35	G0III	2.2	0.6
HR 6467			BD+48 2506	157373	46651						17 20 33.6	+48 11 18	6.43	F4V
HR 6469			BD+40 3136	157482	46664			S		V819 Her	17 21 43.6	+39 58 28	5.51	F9Vn: e		0.0	D:Recognized as triple system by speckle interferometry: single star G5IV and close pair of which the brighter component,D:is F7V eclipsing, sep. 0.045".,S:Also classified F7V?+G5IV. Weak H alpha emission.,SB:5.53y.,VAR:E, amp. 0.085V, 2.2299d. Also long period var. outside eclipse, amp. 0.04V, 83.2d; probably the rotation period of,VAR:the G5IV component.
HR 6480		73	BD+23 3100	157728	85062	3383				8606	17 24 06.6	+22 57 37	5.74	F0IV			VAR:Delta Sct?
HR 6481			BD+16 3174	157740	102805						17 24 31.5	+16 18 04	5.71	A3V			G:Sirius group?
HR 6482			BD+15 3179	157741	102806				10528		17 24 33.8	+15 36 22	6.35	B9V	4.3	3.9	D:Fixed sep. Companion A6V, optical.
HR 6484	ρ	75	BD+37 2878	157778	66000				10526 B		17 23 40.7	+37 08 48	5.47 H	A0Vn	1.0	4.2	D:Binary with HR 6485, q.v. Another companion with sep. 0.29" seen on 1981.47 (McAlister and Hartkopf). Unresolved on,D:1985.25 (Bonneau et al.).,DYN:0.010".
HR 6485	ρ	75	BD+37 2878	157779	66001				10526 A	8605	17 23 41.0	+37 08 45	4.52 H	B9.5III	1.0	4.2	D:Binary with HR 6484. Combined colors. Combined mag. 4.17V.,DYN:0.010".,S:Silicon star.,VAR:ADS 10526A, E?
HR 6488			BD+38 2928	157853	66006				10531		17 24 02.2	+38 34 58	6.49	F8IV	0.1	0.1	D:dF7, CPM, sep. 0.100". Measured sep. 0.069" on 1985.5 by speckle interferometry.
HR 6491			BD+37 2882	157910	66014				10535		17 24 27.1	+36 57 07	6.28	G5III+F0V	3.6	33.2	D:F0V, CPM.
HR 6495			BD+17 3241	157967	102819		I	W		V640 Her	17 25 54.4	+16 55 03	5.98	M4IIIab	7.5	23.1	VAR:Lb 5.98 - 6.21V.
HR 6499			BD+27 2809	158067	85080	3387		W			17 26 00.9	+26 52 44	6.41	A5IV	5.0	49.4
HR 6502			BD+20 3481	158148	85095	3388					17 26 49.1	+20 04 51	5.54	B5V
HR 6506			BD+34 2971	158261	66054	3389					17 26 46.2	+34 41 45	5.94	A0V			SB:5.9182d, K 25.1k/s, V0 -22.7k/s, asini 2.04.
HR 6509		77	BD+48 2517	158414	46723	650					17 26 44.2	+48 15 36	5.85	A4V
HR 6526	λ	76	BD+26 3034	158899	85163	1460	I			9070	17 30 44.3	+26 06 38	4.41	K3.5III			N:Maasym; Masym; Misam, a name also applied to h and Chi Per.
HR 6528			BD+31 3047	158974	66103						17 30 55.4	+31 09 30	5.61	G8III
HR 6531			BD+39 3147	159026	66102						17 30 40.3	+38 52 56	6.43	F6III
HR 6533		78	BD+28 2767	159139	85182						17 31 49.6	+28 24 27	5.62 R	A1V
HR 6538			BD+34 2989	159222	66118						17 32 01.1	+34 16 15	6.56	G5V			G:Theta Cen group.
HR 6541			BD+19 3354	159332	102912	3393					17 33 22.8	+19 15 24	5.64	F6V
HR 6542			BD+16 3218	159353	102917	3394					17 33 39.4	+16 19 03	5.69	gK0
HR 6543			BD+14 3279	159354	102918		I			V642 Her	17 33 42.8	+14 50 30	6.48	M4IIIa			VAR:SRb 6.41 - 6.56V, about 12d.
HR 6550			BD+41 2850	159501	46792	1462					17 33 07.3	+41 14 37	5.74	gK1
HR 6551			BD+16 3220	159503	102928						17 34 27.2	+16 30 14	6.40 R	A8Vn
HR 6559			BD+21 3157	159834	85232				10655		17 35 59.6	+20 59 46	6.10	A7IV	3.5	10.4	D:Companion, 9.53V, +0.36(B-V), -0.02(U-B), F6IV-V, CPM.
HR 6563			BD+37 2908	159925	66165	3395					17 35 42.4	+37 18 06	6.10	G9III
HR 6564			BD+28 2787	159926	85236						17 36 07.9	+28 11 05	6.38 R	K5
HR 6570			BD+30 3033	160054	66175	3397					17 36 36.7	+30 47 07	6.02	A5V
HR 6571		79	BD+24 3218	160181	85264	3400		S			17 37 31.1	+24 18 36	5.77	A2Vn		0.1
HR 6574		82	BD+48 2542	160290	46838		I				17 36 37.6	+48 35 08	5.37	gK1
HR 6579			BD+32 2964	160507	66214						17 38 49.7	+32 44 22	6.37 R	gG5
HR 6584			BD+31 3075	160677	66231		I				17 39 57.5	+31 12 09	6.03	M2IIIab
HR 6588	ι	85	BD+46 2349	160762	46872	663		W		Iot Her	17 39 27.9	+46 00 23	3.80	B3IV	8.3	116.0	C:Color excess E(B-V) = -0.02.,SB:113.804d, K 5.4 k/s, V0 -20.0 k/s, asini 7.629. RV also var. 0.1434d.,VAR:Beta C?, amp. 0.01V.
HR 6589			BD+15 3246	160765	103020						17 41 11.0	+15 10 41	6.34	A1V
HR 6591			BD+31 3076	160822	66243			W			17 40 41.2	+31 17 15	6.28	K0III	2.1	115.0
HR 6592			BD+24 3225	160835	85310				10715		17 41 05.5	+24 30 48	6.36	K1III+F4V	3.0	16.3	D:Component B, F4V CPM.
HR 6594			BD+16 3256	160910	103033				10723		17 41 58.7	+15 57 07	5.52	F4V w	2.8	0.6	D:AB 5.58 F4V, 11.1, 122.68y, a = 1.004". Component C, 12.8v at 155" CPM.,DYN:0.030".
HR 6599			BD+43 2781	160950	46883						17 40 37.6	+43 28 15	6.59 R	K2
HR 6602		83	BD+24 3231	161074	85344		I	W			17 42 28.4	+24 33 51	5.52	K4III	3.6	159.6
HR 6604			BD+14 3321	161149	103052	3407					17 43 22.0	+14 17 42	6.24	F5II			G:Hyades group.,S:Also classified F4IV, Sr enhanced; F2III and F4V.,VAR:Delta Sct?
HR 6608		84	BD+24 3237	161239	85360						17 43 21.6	+24 19 40	5.71	G2IIIb
HR 6611			BD+14 3329	161321	103069				10749	V624 Her	17 44 17.3	+14 24 37	6.19	A3m	5.7	39.7	D:Visual companion ADS 10749B, optical.,S:Also classified A3pSiSr and A2.5/A7/F0.,SB:ADS 10749A, 3.894977d, K 96.6k/s, V0 -32.4k/s, msin3i 1.83, asini 5.17. Both components Am. vsini 35 and 30k/s.,VAR:EA 6.18 - 6.36V, 3.894977d.
HR 6612			BD+44 2757	161369	46906	3408	I				17 43 05.6	+44 05 04	6.34	K4III
HR 6619			BD+31 3090	161695	66311	3410					17 45 40.3	+31 30 17	6.23	A0Ib
HR 6623	μ	86	BD+27 2888	161797	85397	667	I		10786		17 46 27.5	+27 43 14	3.42	G5IV	6.4	33.8	D:BC 10.3 dM4, 10.8, 43.20y, a = 1.360". This close pair forms a wider physical binary with component A.,DYN:0.132".,G:Wolf 630 group.
HR 6625			BD+38 2997	161815	66315	3411					17 45 53.7	+38 52 53	6.52	K0
HR 6626			BD+39 3219	161832	66317				10782	V826 Her	17 45 58.5	+39 19 21	6.68	K3III+F7V	3.1	7.9	D:Component B, 9.70V, +0.75(B-V), +0.19(U-B), F5V, binary. Component C mag. diff 5.36v at 70" from A.,SB:ADS 10782A, 99.557d, K 16.45k/s, V0 -26.72k/s, asini 22.52.
HR 6627			BD+17 3334	161833	103106				10795		17 47 08.0	+17 41 50	5.72 R	A1V	1.3	0.6	D:Binary.
HR 6638			BD+20 3570	162076	85429	1465					17 48 24.8	+20 33 56	5.69	G5IV
HR 6641			BD+47 2537	162132	46954			S			17 47 08.1	+47 36 44	6.43	A2V s		0.1	SB:2.8242d, K 60.2k/s, V0 -27.1k/s, asini 2.34.
HR 6642			BD+19 3435	162161	103131						17 48 47.9	+19 15 19	6.12	A1V
HR 6644		87	BD+25 3353	162211	85437	3415	I				17 48 49.2	+25 37 22	5.12	K2III
HR 6654			BD+29 3126	162555	85464						17 50 22.9	+29 19 20	5.50	K1III
HR 6655			BD+22 3227	162570	85468						17 50 48.4	+22 18 59	5.98 R	A9V
HR 6664		88	BD+48 2581	162732	46997	3417				V744 Her	17 50 03.3	+48 23 39	6.68	BepShell v			S:H alpha emission.,SB:86.59d, K 9.7k/s, V0 -11.6k/s, asini 11.4. Companion 1 solar mass at about 150 solar radii.,VAR:Gamma Cas 6.65 - 6.94V, 86.7207d, similar to Pleione (HR 1180). Spectrum var. with possible periods 2.5552 and,VAR:0.78906d, correlated with RV.
HR 6665			BD+15 3292	162734	103161				10850		17 51 58.5	+15 19 33	6.46 R	K0III	0.2	0.8	D:AB binary. C, 13v at 28" and D, 10v at 95" both optical.,G:Probable Hyades group.
HR 6669			BD+40 3225	162826	47009						17 51 14.0	+40 04 21	6.46 R	G0V
HR 6673			BD+40 3228	162989	66402	3419	I				17 52 04.7	+39 58 56	6.04	gK4
HR 6674			BD+46 2379	163075	47023						17 52 01.0	+46 38 36	6.38	K0III
HR 6677		90	BD+40 3233	163217	47037		I		10875	9834	17 53 18.1	+40 00 29	5.16	K1IIIbCN-1	3.3	1.6	DYN:0.003".,G:Hyades group.,S:If the secondary is a main sequence star, the inferred spectral type is A5V.,VAR:ADS 10875. Not certain which component is the var. suspect. Rapid change in difference between components.
HR 6685		89	BD+26 3120	163506	85545	1468	I			V441 Her	17 55 25.2	+26 03 00	5.46	F2Ib e			C:IR excess.,RV:About 70d. Mass loss 10E-08 solar masses/y.,S:2- and 10-micrometer spectra show silicate emission indicating circumstellar shell. Infrared emission at wavelengths,S:longer than 2 micrometers probably originates in circumstellar shell of solid particles.,VAR:SRd 5.34 - 5.54V, 68:d.
HR 6687			BD+22 3237	163547	85552	3427	I				17 55 50.8	+22 27 51	5.58	gK3
HR 6695	θ	91	BD+37 2982	163770	66485	672	I			9890	17 56 15.2	+37 15 02	3.86	K1IIaCN+2 e			VAR:Possibly 5 yr. period in He 10830 emission.
HR 6697			BD+24 3283	163840	85575			S			17 57 14.3	+23 59 45	6.30	G2V	1.5	0.1	D:Sep. 0.107". Closed from 0.114" to 0.065" between 1981.5 and 1984.3 (McAlister and Hartkopf). However, speckle,D:observations 1986.44 (Blazit et al. 1987, A&AS, 71, 57) yield 0.085".,M:Possible nearby star on basis of spectroscopic parallax.
HR 6702			BD+45 2627	163990	47080		I			OP Her	17 56 48.4	+45 21 03	6.02	M5IIbS			S:Technetium star.,VAR:SRb 5.85 - 6.73V, 7.7 - 8.3p, 120.5d.
HR 6703	ξ	92	BD+29 3156	163993	85590	674	I			9927	17 57 45.9	+29 14 52	3.70	G8+III
HR 6707	ν	94	BD+30 3093	164136	66524					Nu Her	17 58 30.2	+30 11 22	4.41	F2II			S:Manganese star. IUE observations suggest B9.5V companion.,VAR:SRd? 4.38 - 4.48V, 29:d. However, more recent photoelectric observations cast doubt on variability.
HR 6711			BD+36 2986	164280	66531						17 58 42.3	+36 17 16	6.00	gG5
HR 6713		93	BD+16 3335	164349	103285	1469	I				18 00 03.4	+16 45 03	4.67	K0.5IIb			G:Red star Pleiades group.,S:Barium star.
HR 6718			BD+45 2635	164429	47106					V771 Her	17 58 52.3	+45 28 34	6.48	B9pSiSr			VAR:Alpha CV 6.44 - 6.52V, amp. 0.04U, 0.517468d.
HR 6720			BD+19 3494	164447	103291					Var?	18 00 27.7	+19 30 21	6.50	B8Vne			S:Shell star.
HR 6722			BD+15 3327	164507	103299						18 00 57.2	+15 05 36	6.26	G5IV
HR 6726			BD+33 3006	164614	66551		I				18 00 36.4	+33 12 50	5.99	gK6
HR 6728			BD+45 2638	164646	47121	3433	I			9980	17 59 56.2	+45 30 05	5.67	M0IIIab
HR 6729		95	BD+21 3280	164668	85647		I		10993 B	10014	18 01 29.9	+21 35 43	5.18	G8III	0.1	6.3	D:Binary with 6730.,DYN:0.007".
HR 6730		95	BD+21 3280	164669	85648				10993 A	10014	18 01 30.4	+21 35 44	4.96	A5IIIn	0.1	6.3	D:Binary with 6729.,DYN:0.007".
HR 6737			BD+33 3009	164824	66562	3434	I		10998		18 01 35.9	+33 18 41	6.15	K5III	6.0	14.2	D:AB CPM. C, 13v at 55" optical.
HR 6738		96	BD+20 3649	164852	85672					V820 Her	18 02 23.1	+20 50 01	5.28	B3IV			RV:12.7d.,SB:12.4573d, K1 57.6k/s, K2 57.5k/s, V0 -15.5k/s, m1sin3i 0.591, m1sin3i 0.592,,SB:a1sin3i 12.0, a2sin3i 12.0.,VAR:5.17 - 5.19B. Observations satisfy the SB period.
HR 6741		97	BD+22 3260	164900	85676						18 02 30.1	+22 55 23	6.21	B3Vn
HR 6744			BD+19 3508	165029	103334						18 03 14.7	+19 36 47	6.50 R	A0V
HR 6753			BD+48 2627	165358	47173				11028		18 03 09.0	+48 27 52	6.21	A2V	2.7	26.8	D:Both companions optical.
HR 6754			BD+23 3254	165373	85706						18 04 40.2	+23 56 33	6.34	F0IV-V
HR 6763			BD+21 3300	165524	85718						18 05 30.2	+21 38 49	6.15	gK3
HR 6764			BD+40 3276	165567	47193						18 04 43.2	+40 05 03	6.52	F7V
HR 6765		98	BD+22 3273	165625	85725		I			10208	18 06 01.9	+22 13 08	5.06	M3-IIIZrO 0+
HR 6767			BD+41 2968	165645	47195				11054		18 05 00.8	+41 56 48	6.34	F0V	3.6	23.4
HR 6768			BD+32 3047	165683	66626						18 05 49.6	+32 13 50	5.71	K0III
HR 6775		99	BD+30 3128	165908	66648				11077		18 07 01.5	+30 33 43	5.04	F7V	3.4	1.7	D:AB 5.10 F7V, 8.50 K4V, 55.8y, a = 1.00".,DYN:0.060".,S:Metal deficient, calcium rich.,SB:Astrometric binary unresolved by speckle interferometry.
HR 6779	ο	103	BD+28 2925	166014	85750	681		S		Omi Her	18 07 32.6	+28 45 45	3.83	B9.5V e			S:H alpha emission.,VAR:Gamma Cas 3.81 - 3.9B, 4.1 - 4.2p.
HR 6781		100	BD+26 3178	166045	85753				11089 A	10253	18 07 49.5	+26 06 05	5.86	A3V	0.0	14.3	D:Binary with HR 6782. Primary is speckle binary, sep. 0.106". Component C, 11v at 76". A companion to A at 0.106",D:discovered by speckle interferometry.,VAR:Combined light of 6781-2 varies; uncertain which component the variable.
HR 6782		100	BD+26 3178	166046	85752				11089 B	10253	18 07 49.5	+26 05 51	5.90	A3V	0.0	14.3	D:Binary with HR 6781.
HR 6787		102	BD+20 3674	166182	85769	3443			11102		18 08 45.5	+20 48 52	4.36	B2IV	7.9	23.4	D:Companion A6V, optical.
HR 6791			BD+43 2892	166208	47237		I				18 07 28.8	+43 27 42	5.00	G8IIICN-1CH-3
HR 6792			BD+49 2732	166228	47233				11090		18 07 06.3	+49 42 38	6.32 R	A2V	4.1	2.4
HR 6793			BD+36 3027	166229	66666		I				18 08 02.2	+36 24 05	5.48	K2.5III
HR 6794		101	BD+20 3675	166230	85770						18 08 52.9	+20 02 43	5.10	A8III
HR 6799			BD+30 3138	166411	66682						18 09 10.2	+30 28 10	6.38	gK1
HR 6803			BD+16 3390	166479	103443				11123	10311	18 10 08.7	+16 28 36	6.09 R	B9V+F7III	0.8	1.2	D:6.5 A, 7.2 F2, 3040y, a = 1.500".,S:Also classified G2III + A0V:.
HR 6806			BD+38 3095	166620	66700					10316	18 09 37.5	+38 27 27	6.40	K2V			G:Wolf 630 group.
HR 6807			BD+36 3039	166640	66703						18 09 59.0	+36 27 59	5.58	G8III
HR 6814			BD+33 3044	166988	66733				11149	10363	18 11 45.1	+33 26 49	5.88 R	A3V	0.3	0.1	D:AB measured sep. 0.102" on 1985.5 by speckle interferometry.,SB:ADS 11149A.,VAR:ADS 11149B, 8.5 - >11?v.
HR 6815		104	BD+31 3199	167006	66737	3448	I			V669 Her	18 11 54.2	+31 24 19	4.97	M3III			VAR:Amp. 0.14B.
HR 6820			BD+21 3347	167193	85836		I				18 13 16.5	+21 52 49	6.12	K4III
HR 6824			BD+41 3011	167304	47305						18 12 42.6	+41 08 49	6.36	K0III
HR 6826			BD+38 3113	167370	66765	3451					18 13 04.8	+38 46 25	6.04	B9IIIn
HR 6831			BD+29 3213	167588	85856						18 14 44.0	+29 12 26	6.56	F8V
HR 6852			BD+18 3623	168270	103581						18 18 07.7	+18 07 53	5.99 R	B9V
HR 6854			BD+23 3299	168323	85906		I	W			18 18 07.7	+23 17 48	6.63 R	K5	2.3	155.4
HR 6860		105	BD+24 3381	168532	85921	3457	I				18 19 10.7	+24 26 46	5.27	K3III:Ba0.4			SB:478d, K 16.1k/s, V0 -14.4k/s, asini 97.0.
HR 6867			BD+29 3236	168694	85933		I				18 19 52.1	+29 39 58	5.99	gK4
HR 6868		106	BD+21 3390	168720	85941		I				18 20 17.9	+21 57 41	4.95	M1III
HR 6876		108	BD+29 3241	168913	85956						18 20 57.1	+29 51 32	5.63	A5m			SB:5.5146d, K 70.1k/s, V0 -20.2k/s, msin3i 1.72, asini 5.32. vsini both components 20k/s.
HR 6877		107	BD+28 2981	168914	85957					10690	18 21 01.0	+28 52 12	5.12	A7V
HR 6882			BD+23 3316	169110	85975		I				18 22 08.7	+23 17 07	5.41	M0IIIab
HR 6885			BD+17 3555	169191	103655	3460	I				18 22 49.0	+17 49 36	5.25	K3III
HR 6887			BD+16 3478	169223	103660						18 23 02.9	+16 41 17	6.22	K0
HR 6895		109	BD+21 3411	169414	86003	690	I	W		10742	18 23 41.9	+21 46 11	3.84	K2.5IIIab	6.5	221.8
HR 6904			BD+27 3016	169718	86019				11334		18 24 58.5	+27 23 43	6.27	A0V+A4V	0.9	0.6	D:AB 6.5 A2V, 7.5 A4V, 775y, a = .90".,SB:ADS 11334A.
HR 6906			BD+14 3533	169820	103709			S			18 25 55.4	+14 58 00	6.37	B9V		0.1
HR 6917			BD+29 3259	169981	86043	1479					18 25 58.8	+29 49 44	5.83	A2IV			G:Sirius group; UMa stream.,SB:9.6120d, K 28.5k/s, V0 +7.5k/s, asini 3.32.
HR 6924			BD+26 3259	170111	86060				11356		18 26 40.9	+26 26 58	6.53	B3V	2.7	62.3	D:B, 12.6v at 6". Possibly CPM and common RV with HD 170051, 6.9v B5 at 185".,SB:ADS 11356A.
HR 6943			BD+23 3347	170650	86115						18 29 35.7	+23 51 58	5.90	B6IV
HR 6950			BD+20 3821	170829	86142					Var?	18 30 41.6	+20 48 55	6.50	G8IV			SB:26.390d, K 12.4k/s, V0 -59.0k/s, asini 4.43.
HR 6955			BD+16 3529	170878	103800	1481					18 31 04.4	+16 55 43	5.77	A2V
HR 6966			BD+23 3363	171245	86175	3472	I	W			18 32 46.2	+23 37 01	5.84	gK5			D:Suspected binary probably single star.
HR 6975			BD+20 3847	171487	86203	3476					18 34 19.6	+20 27 59	6.57	A3V
HR 6977			BD+18 3740	171623	103879			S			18 35 12.6	+18 12 12	5.78 R	A0Vn		0.2
HR 6980			BD+23 3385	171745	86224				11479		18 35 30.4	+23 36 20	5.61	G9III+G7III	0.2	0.6	D:6.3 G9III, 6.5 G7III, 210.9y, a = 0.416" or 190.8y, a = 0.418". Combined mag., colors.
HR 6981			BD+16 3560	171746	103886				11483	11085	18 35 53.2	+16 58 32	6.21	G2V+G2V	0.2	1.8	D:AB 6.8 G2V, 7.0 G2V, 292y, a = 1.358", or 3083y, a = 6.7811".,DYN:0.024".,S:AB also classified F8V.
HR 6995			BD+16 3563	171994	103913						18 37 09.0	+16 11 54	6.29	G8IV
HR 7047			BD+23 3439	173494	86393						18 44 40.2	+23 35 23	6.31	F6V
HR 7058			BD+21 3550	173650	86405					V535 Her	18 45 35.7	+21 59 06	6.51	B9pSiCr: v			S:Si star. Enhanced chromium, iron, titanium, strontium.,VAR:Alpha CV 6.41 - 6.58V, 10.1353d or 9.975d; also spectrum, magnetic field, RV.
HR 7061		110	BD+20 3926	173667	86406	703	I		11658	11323	18 45 39.7	+20 32 47	4.19	F6V	9.2	63.8	D:All companions probably optical.
HR 7067			BD+18 3817	173833	104087		I				18 46 41.4	+18 42 21	6.17	K5
HR 7069		111	BD+18 3823	173880	104093	1491		W			18 47 01.3	+18 10 53	4.36	A5III	5.5	121.3	G:Hyades group.
HR 7079			BD+23 3461	174160	86451						18 48 16.4	+23 30 51	6.15	F8V			M:Possible nearby star on basis of spectroscopic parallax.
HR 7086			BD+19 3798	174262	104129						18 48 53.4	+19 19 43	5.88	A1V
HR 7091			BD+24 3545	174369	86462			S			18 49 14.4	+25 02 47	6.59 R	A1V		0.2	SB:13.081d, K 28.9k/s, V0 -25.9k/s, asini 4.79.
HR 7109			BD+13 3787	174853	104196	3503		S		V822 Her	18 52 01.9	+13 57 56	6.14	B8Vnn		0.1	S:nn spectral type probably due to unresolved double lines on classification plates (Hube et al. 1988, AJ, 95, 199).,S:Spectral type of secondary similar to that of primary (late B). vsini of primary and secondary 96 and 91k/s,,S:respectively.,SB:1.391113d, K 165.8k/s, V0 -24.1k/s, msin3i 2.63, asini 3.17.,VAR:EB 6.12 - 6.30V.
HR 7113		112	BD+21 3582	174933	86521						18 52 16.4	+21 25 31	5.48	B9II-IIIpHg			G:Possible Pleiades group.,S:HgMn star. Spectrum shows phosphorus. Gallium II lines strong.,SB:6.3624d, K 17.7k/s, V0 -19.6k/s, asini 1.54.
HR 7133		113	BD+22 3524	175492	86567	3508	I		11820		18 54 44.9	+22 38 42	4.59	G4III+A6V	7.9	35.7	D:C, 11v at 38" optical.,S:Also classified G5III + A2V.,SB:ADS 11820A, 245.3d, K 16.0k/s, V0 -23.3k/s, asini 53.6. Binary motion corresponds to the G-type spectrum; the A,SB:type arises from an unresolved companion, vsini 60k/s.
HR 7147			BD+17 3778	175744	104271					V828 Her	18 56 03.9	+17 59 42	6.63	B9pSi			G:Member of Pleiades group.
HR 7148			BD+17 3779	175743	104272						18 56 06.2	+18 06 19	5.69	K1III			G:Gamma Leo group.

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

Hercules / Yale Bright Star Catalog (HR)

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