Catalogues

Catalogue

Constellation

Andromeda / 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 1			BD+44 4550	3	36042				46		00 05 09.9	+45 13 45	6.70	A1Vn	4.2	21.6
HR 8			BD+28 4704	166	73743				69	33	00 06 36.8	+29 01 17	6.13	K0V	2.6	158.6	VAR:6.09 - 6.14V.
HR 15	α	21	BD+28 4	358	73765	1	I		94	Alp And	00 08 23.3	+29 05 26	2.06	B8IVpMnHg v	8.5	81.5	G:Pleiades group.,N:ALPHERATZ; Alpherat; Sirrah; Sirah. Also formerly called Delta Peg.,R:Radius 5 solar.,S:Gallium II lines strong. HgMn star. Spectrum appears earlier at shorter wavelengths.,SB:ADS 94A, 96.6960d, K 30.8k/s, V0 -11.6k/s, asini 34.2.,VAR:Alpha CV 2.02 - 2.06V, 0.9636 or 0.966222d. Some spectral lines vary same period, others half period, some nonvariable.
HR 17			BD+35 8	400	53677						00 08 41.0	+36 37 36	6.19	F8IV
HR 27		22	BD+45 17	571	36123	4					00 10 19.3	+46 04 20	5.03	F2II			G:In neutral hydrogen region.
HR 36			BD+47 21	743	36148		I				00 11 59.1	+48 09 09	6.16	gK4
HR 38			BD+36 12	829	53725						00 12 50.4	+37 41 36	6.73	B2V			G:Cas-Tau OB1.
HR 40			BD+26 13	895	73823				161		00 13 24.0	+26 59 14	6.30	G0III	1.1	0.1	D:AB 6.7 G3III, 7.5 F2IV, 368y, a = 0.564". ADS 161C, 10.37V, K0, at 18", physical.,DYN:0.0065".,S:Combined spectrum variously classified as F7V, G0V, G0III.
HR 41		23	BD+40 29	905	36173	2010					00 13 30.8	+41 02 07	5.72	F0IV
HR 44			BD+32 21	952	53744	2012					00 14 02.3	+33 12 22	6.25	A1V
HR 52			BD+30 26	1075	53755		I				00 15 07.0	+31 32 09	6.45 R	K5
HR 53			BD+26 23	1083	73842			W			00 15 10.6	+27 16 59	6.35	A1Vn	6.8	29.2	SB:Published RV range from -75 to +14k/s.
HR 56			BD+42 41	1185	36221				215		00 16 21.6	+43 35 41	6.15	A2VpSi	3.9	9.2	D:CPM.
HR 63	θ	24	BD+37 34	1280	53777					116	00 17 05.5	+38 40 54	4.61	A2V			G:Possible Eggen group with V = +5k/s. Other members: HR 118, 378, 1046, 1706, 2375, 2572, 3131, 3894, 4564, 5482, 5843,,G:6153, 6250, 6355, 6446, 7102, 7124, 7340, 8709.
HR 68	σ	25	BD+35 44	1404	53798	1005				118	00 18 19.7	+36 47 07	4.52	A2V			G:Sirius group; UMa stream.,VAR:Delta Sct?, 4.49 - 4.55V.
HR 70		26	BD+42 48	1438	36256				254	119	00 18 42.1	+43 47 28	6.11	B8V	4.1	6.2	D:CPM. Companion F3V.,VAR:ADS 254B, 9.5 - 12v.
HR 71			BD+30 35	1439	53803	1006					00 18 38.3	+31 31 02	5.87	A0IV
HR 75			BD+39 56	1527	36269						00 19 41.6	+40 43 47	6.33	K1III
HR 78			BD+30 42	1606	53820					128	00 20 24.4	+30 56 09	5.90	B7V
HR 79			BD+32 45	1632	53825		I				00 20 45.5	+32 54 41	5.79	K5III
HR 82	ρ	27	BD+37 45	1671	53828	1009					00 21 07.3	+37 58 07	5.18	F5III
HR 90			BD+37 58	1967	53860		I	W		R And	00 24 02.0	+38 34 38	7.39	S6.5IIIeZr6Ti2	4.9	84.6	S:CO emission. Technetium star, also classified S6.5IIIe, S4/4eZr6Ti2, and S3,5e - S8,8e (M7e).,VAR:M 5.8 - 14.9v, 409.33d.
HR 104			BD+43 92	2421	36390	2027					00 28 13.7	+44 23 40	5.17	A2V s			SB:3.9558d, K 41.7k/s, V0 +2.0k/s, asini 2.24.
HR 110			BD+36 66	2507	53928						00 28 56.6	+36 54 00	6.26	G5III
HR 114		28	BD+28 75	2628	74041				409	GN And	00 30 07.3	+29 45 06	5.23	A7III	7.1	139.3	D:ADS 409B 13.3v at 3" CPM with A.,S:Spectrum classified variously as Am, A7III, F0III, F2V.,VAR:Delta Sct 5.18 - 5.22V, 0.0689797d.
HR 122			BD+32 80	2767	53956			W			00 31 25.6	+33 34 54	5.87	K1III	2.4	56.4
HR 128			BD+42 99	2888	36453						00 32 26.8	+43 29 41	6.70	A1Vn			S:Also classified A0pSi.
HR 133			BD+26 76	2924	74083						00 32 34.5	+27 34 50	6.67	A2IV
HR 134			BD+27 84	2942	74090				455		00 32 49.1	+28 16 49	6.30	K0III	4.9	8.5	D:ADS 455AB, CPM. B, 10.4v K0V. C, 12.3v at 60".,SB:ADS 455A.
HR 149			BD+26 91	3322	74136					221	00 36 20.0	+27 15 17	6.50	B8IIIpHgMn:			SB:Probable SB with period about 400d.,VAR:Amp. 0.06B.
HR 152			BD+43 113	3346	36509		I				00 36 46.6	+44 29 19	5.13	K5-M0III
HR 154	π	29	BD+32 101	3369	54033	18			513	227	00 36 52.9	+33 43 10	4.36	B5V	4.2	35.2	D:AB 103000?y. Component B spectrum A6V or Am(A3/F0/F2), RV +11.9k/s. Component C, 11.4v, F3 at 55" optical.,RV:The secondary has evidently been seen only by J. A. Pearce in 1936.,SB:ADS 513A, 143.6065d, K 47.5k/s, V0 +8.35k/s, msin3i 27.1, asini 77.6. Unresolved by speckle interferometry.
HR 156			BD+23 84	3411	74148						00 37 07.2	+24 00 51	6.47 R	K2III
HR 157			BD+34 86	3421	54038						00 37 21.1	+35 23 58	5.48	G2.5IIa
HR 163	ε	30	BD+28 103	3546	74164	19	I				00 38 33.3	+29 18 42	4.37	G6IIIFe-3CH1
HR 165	δ	31	BD+30 91	3627	54058	20	I		548		00 39 19.7	+30 51 39	3.27	K3III	8.2	28.7	D:AB CPM. Component C, 15.2v at 48" optical.,SB:ADS 548A, 15,000d, K 4.0k/s, V0 -8.5k/s, asini 785. Unresolved by speckle interferometry 1983.93.
HR 175		32	BD+38 90	3817	54079	2043					00 41 07.2	+39 27 31	5.33	G8III			G:UMa stream.
HR 178			BD+23 94	3883	74200	2044		W		258	00 41 36.0	+24 37 45	6.04	A7m			D:Suspected visual double is probably single. Resolved by speckle interferometry 1983.93, sep. 0.145", but unresolved,D:1981.68, 1983.94.
HR 205			BD+44 160	4335	36640						00 46 10.9	+44 51 41	6.05	B9.5IIIpHgMnCr			SB:Period at least 2500d.
HR 215	ζ	34	BD+23 106	4502	74267	27	I	W		Zet And	00 47 20.3	+24 16 02	4.06	K1IIe	5.6	162.7	D:AB CPM. Companions probably optical.,S:CaII emission.,SB:Component A of visual system, 17.7692d, K 26.3k/s, V0 -23.7k/s, asini 6.43. Possible X-ray source 3U0032+24.,VAR:Component A of visual system, EB 3.92 - 4.14V, 17.7695d.
HR 226	ν	35	BD+40 171	4727	36699	1021					00 49 48.8	+41 04 44	4.53	B5V+F8V			SB:4.2828d, K 75.6k/s, V0 -23.9k/s, msin3i 1.49, asini 4.45; vsini of secondary 11k/s.
HR 234			BD+44 176	4778	36702	2055				GO And	00 50 18.3	+45 00 08	6.15	A0pCr v			S:Possible subdwarf. CrII, MgII, TiII, SrII, EuII but no trace of SiII.,VAR:Alpha CV 6.10 - 6.14V, 2.156d. Also var. K-line, same period.
HR 246			BD+37 159	5066	54225						00 52 53.4	+38 32 55	6.69	A2V
HR 249			BD+36 148	5118	54237						00 53 28.2	+37 25 05	6.06	gK3
HR 258		36	BD+22 146	5286	74359				755	343	00 54 58.0	+23 37 42	5.47	K1IV	0.4	0.6	D:AB 6.02 G6IV, 6.41 K6IV, 164.68y, a = 1.014". Resolved by speckle interferometry 1983.94, sep. 0.68". Combined,D:mag., colors.
HR 269	μ	37	BD+37 175	5448	54281	33			788		00 56 45.2	+38 29 58	3.87	A5V	6.8	266.7	D:All components optical.
HR 271	η	38	BD+22 153	5516	74388	2060	I	W			00 57 12.4	+23 25 03	4.42	G8IIIb	6.9	131.7	G:UMa stream.,SB:115.71d, K 17.9k/s, V0 -10.3k/s, msin3i 0.338, asini 28.5; both components vsini <17k/s.
HR 272			BD+45 237	5526	36795						00 57 39.7	+45 50 23	6.12	K2III
HR 275			BD+33 140	5608	54306	2061					00 58 14.2	+33 57 03	5.98	K0
HR 282			BD+43 193	5788	36832				824 B		01 00 03.4	+44 42 40	6.84 H	A2Vn	0.8	7.8	D:Visual binary with HR 283.
HR 283			BD+43 193	5789	36833				824 A		01 00 03.6	+44 42 48	6.04 H	B9.5Vn	0.8	7.8	D:Visual binary with HR 282. Color for blended images.
HR 289			BD+46 243	6114	36875				862		01 03 01.5	+47 22 34	6.45	A9IV	1.0	0.9	D:6.7 A3n, 8.0, 450y, a = 0.816".,DYN:0.010".,G:Hyades group.,SB:ADS 862A.
HR 290		39	BD+40 209	6116	36874				863		01 02 54.3	+41 20 42	5.98	A5m	6.2	20.9	G:UMa stream.,S:Also classified A3/A7/A9.
HR 305			BD+39 249	6314	54398						01 04 36.4	+39 59 28	6.72	F0Vn
HR 324		41	BD+43 234	6658	36950	2071					01 08 00.9	+43 56 31	5.03	A3m			G:Hyades group.
HR 335	φ	42	BD+46 275	6811	36972				940	Var?	01 09 30.2	+47 14 31	4.25	B7Ve	1.2	0.4	D:4.6 B6IV, 5.5 B9V, 371.6y, a = 0.447". Combined mag., colors. Masses 16 and 10 solar. Resolved by speckle,D:interferometry 1983.93, sep. 0.64".,DYN:0.003".,S:Also classified B7III, B9IIIe.
HR 337	β	43	BD+34 198	6860	54471	42	I		949	414	01 09 43.9	+35 37 14	2.06	M0+IIIa e	10.1	80.4	N:MIRACH; Merach; Mirac; Mirak; (al Mizar).,S:Ultraviolet FeII emission. Also classified B9III.
HR 340		44	BD+41 219	6920	36984	2075					01 10 18.8	+42 04 53	5.65	F8V
HR 348		45	BD+36 201	7019	54494			W			01 11 10.3	+37 43 27	5.81	B7III-IV	0.0	0.4	D:Unresolved by speckle interferometry: probably single.
HR 355			BD+44 261	7158	37023		I				01 12 34.0	+45 20 16	6.11	M1III
HR 369			BD+47 357	7546	37067	2085					01 16 24.5	+48 04 56	6.61	B9IIIpSi
HR 372			BD+44 271	7647	37077		I				01 17 05.1	+44 54 07	6.34 R	K5
HR 376			BD+46 319	7758	37096						01 18 10.2	+47 25 11	6.25	K0
HR 379			BD+36 220	7853	54592				1055		01 18 47.0	+37 23 10	6.46	A5m	3.1	6.2
HR 390	ξ	46	BD+44 287	8207	37155	1035	I				01 22 20.4	+45 31 44	4.88	K0-IIIb			N:Adhil.,SB:17.7673d, asini 6.272.
HR 395		47	BD+36 237	8374	54655	2093					01 23 40.6	+37 42 54	5.58	A2Vm			G:Hyades group.,SB:35.371d, K 39.0k/s, V0 +13.3k/s, msin3i 0.440, asini 14.7; vsini same for both components 15k/s.
HR 396			BD+33 220	8375	54654						01 23 37.5	+34 14 45	6.29	G8IV
HR 409			BD+42 302	8671	37204						01 26 18.6	+43 27 28	5.96	F7V
HR 410			BD+33 228	8673	54695						01 26 08.7	+34 34 47	6.31	F7V			G:Hyades moving group.
HR 415			BD+33 234	8774	54705						01 27 06.2	+34 22 39	6.27	F7IVb vs			G:Hyades moving group.
HR 417	ω	48	BD+44 307	8799	37228	1040			1152		01 27 39.4	+45 24 24	4.83	F5IV	6.6	119.0	D:AB binary, B 11.7v at 2"; CD 10.4, 10.4 sep. 4.9" at 120" from A.,G:Hyades moving group.
HR 418			BD+40 289	8801	37227				1151		01 27 26.6	+41 06 02	6.46	A7m	5.9	15.3	D:Optical.
HR 422			BD+39 334	8837	37234						01 27 47.0	+40 20 08	6.60	A0III			G:Member of the local association (Pleiades group); in neutral hydrogen region.,RV:Two published values of vsini are 35 and 135k/s.,S:Shell star.
HR 430		49	BD+46 370	9057	37275		I				01 30 06.2	+47 00 26	5.27	K0III
HR 446			BD+36 277	9531	54788					KK And	01 34 16.6	+37 14 14	5.88	B9IV			S:Si star.,VAR:Alpha CV, amp. 0.012V, 0.6684d. Also long-period variations.
HR 452			BD+40 328	9712	37344						01 35 52.5	+41 04 35	6.38	K1III
HR 454			BD+47 460	9746	37351					OP And	01 36 27.2	+48 43 22	5.92	gK1			VARBY, amp. 0.09V. Four minima observed with unequal intervals, about 36 to 66 days superposed on possible secular,VAR:brightening at rate of about 0.045m/100d.
HR 458	υ	50	BD+40 332	9826	37362	1045	I	W			01 36 47.8	+41 24 20	4.09	F8V	8.4	114.0	D:Both visual companions probably optical.,SB:197.9d, K 1.8k/s, V0 -27.7k/s, asini 4.79. Orbit questioned by Morbey and Griffin (1987, ApJ, 317, 343).,SB:Unresolved by speckle interferometry.
HR 464		51	BD+47 467	9927	37375	52	I				01 37 59.6	+48 37 42	3.57	K3-III			N:51 And also called Upsilon Per, but outside IAU boundaries of Perseus.
HR 465			BD+44 341	9996	37393					GY And	01 38 31.7	+45 24 00	6.36	B9pCrEu v			S:Spectra show high uranium to thorium ratio. Promethium doubtful. Anomalously high abundance of heavy elements.,S:1000-fold overabundance for the rare earths, Mo and Nb; 100 for Sr and Zr; lanthanides 100,000 times; uranium a million,S:times more abundant than in solar system.,SB:272.99d, K 11.3k/s, V0 -0.55k/s, asini 37.4.,VAR:Alpha CV 6.27 - 6.41V, 36.5d; Sp. and magnetic field var., 22-24y. UII and PmII lines vary in 6.7 hrs.
HR 469	χ	52	BD+43 343	10072	37406	2112	I				01 39 21.0	+44 23 10	4.98	G8III
HR 476			BD+42 345	10204	37419						01 40 39.8	+43 17 52	5.61	sgA9			G:Hyades moving group.
HR 477	τ	53	BD+39 378	10205	37418				1311	584	01 40 34.8	+40 34 37	4.94	B8III	5.9	52.3	D:CPM. Component B, 11.53V, +0.65(B-V), +0.04(U-B).
HR 483			BD+41 328	10307	37434			A			01 41 47.2	+42 36 49	4.95	G1.5V		0.1	D:Astrometric binary 20y, a 0.12", mag. diff 3-4v. Companion 25% solar mass.,G:Hyades group.
HR 495			BD+44 354	10486	37460						01 43 16.5	+45 19 20	6.34	K2IV			G:61 Cyg group.
HR 504			BD+45 432	10597	37475		I				01 44 26.5	+46 08 23	6.35 R	K5III
HR 518			BD+45 447	10874	37513	2119					01 47 48.0	+46 13 47	6.32	F6V
HR 521			BD+37 372	10975	54991						01 48 38.9	+37 57 10	5.94	K0III
HR 543		55	BD+40 394	11428	37587	2124	I	W			01 53 17.3	+40 43 47	5.40	gK1	5.3	59.8
HR 551			BD+39 434	11613	37607						01 54 53.8	+40 42 07	6.24	K2			SB:838d, K 4.30k/s, V0 +31.89k/s, asini 49.6.
HR 552			BD+36 346	11624	55082		I				01 54 57.5	+37 07 42	6.26	K0
HR 556			BD+36 354	11727	55102		I		1534 B		01 55 54.4	+37 16 40	5.89	gM0	0.2	190.4	D:ADS 1534B not CPM with HR 557, component A.,G:Region of NGC 752.
HR 557		56	BD+36 355	11749	55107				1534 A		01 56 09.3	+37 15 06	5.67	K0III	0.2	190.4	D:ADS 1534AP, CPM, 11.9v at 18".,G:Region of NGC 752.
HR 562			BD+40 407	11905	37653						01 57 56.4	+41 41 40	6.78	B8III			RV:Hydrogen lines show period 5.01d; metallic lines do not. Possible unseen secondary.,S:HgMn star.
HR 603	γ¹	57	BD+41 395	12533	37734	73	I		1630 A		02 03 54.0	+42 19 47	2.26	K3-IIb	2.8	9.6	D:CPM with HR 604.,G:Red star Pleiades group.,N:ALMAAK; Almach; Alamak; Almak; Almaach.
HR 604	γ²	57	BD+41 395	12534	37735				1630 BC		02 03 54.7	+42 19 51	4.84	B8V+A0V	2.8	9.6	D:BC 5.5 B8V, 6.3 A0V, 61.1y, a = 0.296". ADS 1630BC CPM with HR 603. Component D, 15v at 28". Possibly also CPM with,D:BD+41d408 at 53'.,DYN:0.010".,SB:ADS 1630B, 2.67d, K 141k/s, V0 +2.5k/s, msin3i 1.76, asini 4.95; vsini of both components 70k/s.
HR 619			BD+43 431	13013	37794						02 08 33.6	+44 27 34	6.42 R	G8III-IV
HR 620		58	BD+37 486	13041	55289	2145					02 08 29.3	+37 51 33	4.82	A5IV-V
HR 628		59	BD+38 425	13294	55330				1683 A		02 10 52.8	+39 02 22	5.63	B9V	0.8	16.2	D:CPM with HR 629.
HR 629		59	BD+38 425	13295	55331				1683 B		02 10 53.7	+39 02 35	6.10	A1Vn	0.8	16.2	D:CPM with HR 628.
HR 643		60	BD+43 447	13520	37867	2153	I	S		746	02 13 13.3	+44 13 54	4.83	K3.5IIIBa0.5:			SB:748.2d, K4.88k/s, V0 -48.00k/s, asini 47.2.
HR 645			BD+50 481	13530	23047	77		W		747	02 13 36.3	+51 03 57	5.31	G8III: v	4.4	27.3	G:61 Cyg group?,N:6 Per on boundary Per/And.,SB:1650d, K 13.5k/s, V0 +27.3k/s, asini 203. Resolved by speckle interferometry 1981.69, sep. 0.040".
HR 647			BD+46 536	13594	37878				1709		02 14 02.6	+47 29 03	6.06	F4V	0.6	1.0	D:6.6 F3V, 7.08 F6V, 144.7y, a = 0.908". Combined mag., colors.,DYN:0.025".,G:Sirius group; UMa stream.
HR 653			BD+47 590	13818	37905						02 15 57.9	+47 48 41	6.33 R	G9III-IV			G:Probable Hyades group.
HR 663			BD+43 461a	14028	0					W And	02 17 33.4	+44 18 25	6.70	M7-8Se v			M:Proper motion from AGK3. Earlier McCormick determination, +.007",-.002".,S:Also classified S6,1e-S9,2e/M4-M10.,VAR:M 6.7 - 14.6v, 395.93d.
HR 670		62	BD+46 552	14212	37948	1063					02 19 16.8	+47 22 48	5.30	A1V
HR 671			BD+45 589	14213	37947						02 19 10.9	+46 28 21	6.21	A4V
HR 673			BD+48 648	14221	37949						02 19 22.7	+48 57 19	6.37 R	F4V
HR 677			BD+39 521	14272	55453						02 19 37.3	+39 50 06	6.63	B8V
HR 679			BD+46 557	14372	37955						02 20 41.4	+47 18 39	6.11	B5V
HR 682		63	BD+49 640	14392	37960					790	02 20 58.2	+50 09 05	5.59	B9pSi			VAR:Amp. 0.05U, 1.31d.
HR 687			BD+40 500	14622	37986	2161		W			02 22 50.3	+41 23 47	5.82	F0III-IV	1.8	295.5
HR 694		64	BD+49 649	14770	38005		I				02 24 24.9	+50 00 24	5.19	G8III
HR 699		65	BD+49 656	14872	23319	2165	I	W			02 25 37.4	+50 16 43	4.71	K4+III	5.7	191.7
HR 709		66	BD+49 666	15138	23353						02 27 51.8	+50 34 11	6.12	F4V			SB:10.9903d, K 46.5k/s, V0 -5.3k/s, msin3i 0.506, asini 6.91.
HR 746			BD+39 573	16004	55680				1961		02 35 27.9	+39 39 52	6.36	B9pHgMn	5.6	16.3	D:Companions optical.
HR 748			BD+36 519	16028	55684		I		1964		02 35 38.8	+37 18 44	5.71	K3III	5.2	18.3
HR 756			BD+38 515	16176	55705						02 36 57.2	+38 43 58	5.90	F5V
HR 760			BD+39 582	16219	55715						02 37 20.8	+39 53 45	6.54	B5V			SB:2.089920d, K 21.4k/s, V0 +12.0k/s, asini 0.62.
HR 768			BD+37 588	16327	55729				1996		02 38 17.8	+37 43 36	6.18	F6III	5.0	20.8	D:B 12v, 8" optical; AC CPM; D, mag. diff 5.97v at 40" from A.
HR 769			BD+37 591	16350	55735						02 38 27.8	+38 05 22	6.30	B9.5V			S:Also classified A0III.
HR 8744			BD+51 3514	217314	35022	3838	I				22 59 10.3	+52 39 16	6.29	K2
HR 8755			BD+44 4302	217491	52587						23 00 34.4	+45 22 30	6.50	A3V
HR 8758			BD+37 4744	217543	72929					14386	23 00 54.7	+38 42 29	6.54	B3Vpe			G:Lac OB1.,S:Shell star.,VAR:Gamma Cas?, 6.53 - 6.60V.
HR 8762	ο	1	BD+41 4664	217675	52609	869		S		Omi And	23 01 55.3	+42 19 34	3.62	B6IIIpe+A2p v	0.5	0.3	D:Separate speckle interferometric measures give sep. 0.05" (Aa) and 0.34" (AB). Ten years of observations reveal steady,D:change in AB position angle of about 10d with decrease in separation from about 0.375" to 0.266". Component B,D:identified as SB2 (see SB remarks), making total number of components at least 4.,G:In reflection nebula; probably but not certainly associated.,RV:23.5y. vsini about 300k/s.,S:Shell star. Also classified B5III or B6IVpe.,SB:Speckle interferometry indicates triple star. SB periods 72.3145, 8585 or 9478d. Also short period 1.5845, 0.84,,SB:3.66 or 1.67458d, all doubtful. Observations by Hill et al. (1988, PASP, 100, 243) indicate that one of the companions,SB:of A is SB2, and they identify this as component B. Orbit for B: 33.01d, V0 -14.3k/s, K1 54.8k/s, K2,SB:71.6k/s, m1sin3i 3.74, m2sin3i 2.86, a1sini 0.161, a2sini 0.211.,VAR:Gamma Cas 3.58 - 3.65V. Photometric investigations have indicated numerous periods, particularly 0.78823, 1.0815d and,VAR:1.5998398d, all doubtful. Form of light curve varies. Probably not an eclipsing binary. Period shell phenomena about,VAR:23.5y. Shell features have vanished several times since 1897. H gamma varies in 3.66?d.
HR 8766		2	BD+41 4665	217782	52623				16467	14396	23 02 36.3	+42 45 28	5.10	A3Vn	3.7	0.4	D:AB 5.1 A2, 8.8, 76.6y, a = 0.277".,DYN:0.007".,S:Lambda Boo star.,VAR:ADS 16467B, Delta Sct?, 8.7v.
HR 8768			BD+43 4378	217811	52626				16472	LN And	23 02 45.2	+44 03 32	6.39	B2V	3.9	7.4	D:Fixed. Companion 9.88V, +0.08(B-V), -0.37(U-B), A1V.,G:Lac OB1.,VAR:Amp. 0.02b, 35 min.
HR 8780		3	BD+49 4028	218031	52649		I				23 04 11.0	+50 03 08	4.65	K0IIIbFe-0.5
HR 8800			BD+45 4147	218407	52707						23 07 18.1	+46 04 05	6.66	B2V			G:Lac OB1.,SB:3.3378d, K 86.1k/s, V0 -10.3k/s, asini 3.84.
HR 8801			BD+52 3371	218416	35151						23 07 10.1	+52 48 59	6.11	K0III
HR 8804		4	BD+45 4149	218452	52711	3852	I		16526		23 07 39.3	+46 23 14	5.33	K5III	5.5	48.2	G:Sirius group.
HR 8805		5	BD+48 3944	218470	52713	1604					23 07 45.4	+49 17 45	5.70	F5V
HR 8806			BD+43 4399	218525	52717						23 08 12.3	+44 33 42	6.56	A2IV
HR 8825		6	BD+42 4592	218804	52761	3857					23 10 27.2	+43 32 39	5.94	F5IV
HR 8830		7	BD+48 3964	219080	52787						23 12 33.0	+49 24 23	4.52	F0V			SB:Unresolved by speckle interferometry 1986.46.
HR 8837			BD+49 4071	219290	35251						23 14 14.3	+50 37 04	6.31	A0V
HR 8857			BD+44 4368	219668	52865						23 17 16.6	+45 09 51	6.43	K0IV
HR 8860		8	BD+48 3991	219734	52871		I		16656	14484	23 17 44.7	+49 00 55	4.85	M2+IIIBa0.3	5.8	219.4	D:AB, CPM. B, 13.0v at 8".
HR 8861			BD+44 4373	219749	52876					ET And	23 17 56.1	+45 29 20	6.48	B9pSi v			S:Also classified B8Vp.,SB:48.304d, K 25.7k/s, V0 +2.6k/s, asini 14.8. Possible RV fundamental period 140 min. with 70 and 35 min. harmonics.,VAR:Alpha CV 6.48 - 6.50V, larger amp. in U = 0.05, 0.617135d, 0.49925d. Other periods previously determined range from,VAR:0.44925 to 2.604d. Spectral line strengths vary but not in phase with orbital (SB) period.
HR 8864		9	BD+40 5043	219815	52881					AN And	23 18 23.4	+41 46 25	6.02	A7/8Vm			SB:3.219565d, K 71.6k/s, V0 -3.8k/s, asini 3.17. Probable triple system.,VAR:EB 6.0 - 6.16p, A7+A, 3.219565d.
HR 8870			BD+44 4378	219891	52892						23 19 02.4	+45 08 14	6.50	A5Vn
HR 8874		11	BD+47 4110	219945	52907						23 19 29.8	+48 37 31	5.44	K0III
HR 8875			BD+47 4114	219962	52912			W			23 19 41.6	+48 22 51	6.32	K1III	3.3	85.8
HR 8876		10	BD+41 4752	219981	52914	3870	I				23 19 52.4	+42 04 41	5.79	M0III
HR 8884			BD+43 4440	220105	52927				16685		23 20 44.0	+44 06 59	6.13 R	A5Vn	4.0	13.2	D:CPM.
HR 8885		12	BD+37 4817	220117	73190	1610		W			23 20 53.3	+38 10 56	5.77	F5V	3.4	121.1
HR 8902			BD+40 5068	220575	52987						23 24 35.0	+41 06 46	6.72	B8III			S:Hg, Mn.,SB:212.18d.
HR 8913		13	BD+42 4672	220885	53039						23 27 07.4	+42 54 43	5.75	B9III			G:Hyades group.,S:Hg, Mn.
HR 8925			BD+48 4070	221246	53088	3882	I				23 30 07.4	+49 07 59	6.17	K3III			G:NGC 7686 #1.
HR 8927			BD+37 4856	221293	73308						23 30 39.7	+38 39 43	6.05	G9III
HR 8930		14	BD+38 5023	221345	73311		I			14599	23 31 17.4	+39 14 11	5.22	K0III
HR 8941			BD+44 4441	221661	53147						23 33 42.7	+45 03 29	6.24	G8II
HR 8947		15	BD+39 5114	221756	73346	1616				14627	23 34 37.5	+40 14 11	5.59	A1Vp			G:UMa stream.,S:Lambda Boo star, Mg 4481 wk.
HR 8950			BD+37 4866	221776	73351		I		16843		23 34 46.7	+38 01 26	6.18	K7III	5.2	20.2
HR 8955			BD+32 4671	221970	73368						23 36 30.5	+32 54 15	6.35	F6V
HR 8961	λ	16	BD+45 4283	222107	53204	890	I	W		Lam And	23 37 33.9	+46 27 29	3.82	G8III-IV v	6.5	217.6	SB:20.5212d, K 6.6k/s, V0 +6.8k/s, asini 1.86. Radio binary. Unresolved by speckle interferometry. Possible radio,SB:emitter.,VAR:RS 3.69 - 3.97V, 4.74 - 5.13B, 54.20d. Amp. and cycle length vary in period 3200d. Also 0.25m var. in period about,VAR:50d. H and K emission correlated with 56d light period.
HR 8962			BD+43 4508	222109	53202				16877		23 37 32.0	+44 25 45	5.80	B8V	0.9	0.5	D:AB 6.3, 7.2v, 351.22y, a = 0.41".
HR 8964			BD+45 4288	222143	53210						23 37 58.6	+46 11 59	6.58	G5
HR 8965	ι	17	BD+42 4720	222173	53216	891				14646	23 38 08.2	+43 16 05	4.29	B8V
HR 8967		18	BD+49 4180	222304	35642	3897					23 39 08.3	+50 28 18	5.30	B9V
HR 8973			BD+36 5098	222399	73422				16913		23 40 02.8	+37 39 09	6.53	F2IV	4.4	14.9	D:CPM.
HR 8976	κ	19	BD+43 4522	222439	53264	1619			16916		23 40 24.5	+44 20 02	4.14	B9IVn	7.6	46.8	D:AB optical.
HR 8977			BD+35 5074	222451	73428	3899					23 40 40.6	+36 43 15	6.23	F1V			G:Hyades moving group.
HR 8986			BD+44 4473	222641	53292		I			14674	23 42 14.8	+44 59 31	6.57 R	gK5
HR 9003	ψ	20	BD+45 4321	223047	53355	1622	I	W			23 46 02.1	+46 25 13	4.95	G5Ib+A0V	4.0	184.0	D:Component A has composite spectrum but star unresolved by interferometer. vsini of G5 component <19:k/s, A0 component,D:=<50k/s. Component B, 14.6v at 25"; C, 13.1v at 62".
HR 9011			BD+46 4169	223229	53374				17006	14709	23 47 33.2	+46 49 57	6.07	B3IV	2.0	0.9	VAR:ADS 17006. Uncertain which component varies.
HR 9024			BD+35 5110	223460	73535	3914				OU And	23 49 41.0	+36 25 31	5.90	G1III e			S:CaII emission.,VAR:RS CV, amp. 0.04V, 23.25d.
HR 9053			BD+46 4214	224165	53486						23 55 33.6	+47 21 21	6.00	G8Ib
HR 9057			BD+41 4902	224342	53511	3923					23 57 03.6	+42 39 30	5.97	F8III			S:Bidelman classifies gK + F.
HR 9068			BD+31 5012	224544	73650	3927				Var?	23 58 49.2	+32 22 54	6.52	B6IVe			S:Shell star.
HR 9070			BD+45 4381	224559	53540					LQ And	23 58 46.5	+46 24 47	6.54	B4Ven v			G:Cas-Tau OB1.,S:Shell star. Also classified B3IV.,VAR:Beta C? 6.4 - 6.46B, 0.310049 or 0.622832d. Spectrum variable.
HR 9074			BD+32 4747	224635	73656				17149 A		23 59 29.2	+33 43 28	6.58 H	G0V	0.2	1.5	D:AB 6.5 G0V, 6.7 G0V, 355y, a = 3.125". C 12.9V at 82". Blended mag. for HR 9074/5, 5.81V; colors for combined light.
HR 9075			BD+32 4747	224636	73656				17149 B		23 59 29.2	+33 43 28	6.58 H	G0V	0.2	1.5	D:Binary with HR 9074, q.v.
HR 9080			BD+44 4538	224801	53568					CG And	00 00 43.7	+45 15 12	6.38	B9pSiEu v			S:Enhanced Si, Mn, some rare earths. Magnetic star. Also classified A0Vp.,SB:4.88643d. Other RV periods 3.74d or 2.1 hrs. RV hydrogen lines var. per. about 6 hrs.,VAR:Alpha CV 6.32 - 6.42V, 3.73975d, possible cyclical changes. Also magnetic field and spectrum period. Light var. also,VAR:2.1 hrs. Widths of hydrogen lines in about 35 min. SiII var. in per. 4.88643d.
HR 9086			BD+41 4920	224906	53580						00 01 43.8	+42 22 02	6.25	B9IIIpHg:Mn:
HR 9105			BD+41 4933	225218	36037		I		30		00 04 36.7	+42 05 32	6.01 R	B9III	3.7	5.4	D:Binary.,S:Primary discordant classifications, B9III or A3Vs.,SB:ADS 30B, 9.5 F5.
HR 9107			BD+33 4828	225239	53622	2002					00 04 53.8	+34 39 35	6.12	G2V

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

Andromeda / Yale Bright Star Catalog (HR)

Legend

References