Catalogues

Catalogue

Constellation

Perseus / 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 470			BD+53 363	10110	22493		I				01 40 13.1	+53 52 06	6.39	K5III
HR 496	φ		BD+49 444	10516	22554	57	I			Phi Per	01 43 39.6	+50 41 19	4.07	B2Vep			G:In neutral hydrogen region; Cas-Tau OB1.,P:Intrinsic polarization, probably due to circumstellar matter.,S:FeII, H in emission. Also classified B0nne, B1III-Vpe.,SB:126.696d. Primary, 16.8k/s, V0 -8.4k/s, msin3i 21.1, asini 29.2; secondary K 105.3k/s, sin3i 3.4,,SB:asini 184. Unresolved by speckle interferometry. Both components appear to be shell stars, B2Ve and B3Ve. Speculation,SB:that secondary is the helium core of a once more massive star whose mass was transferred to the primary.,VAR:Gamma Cas 4.03 - 4.11V, 19.5d. Amp. varies in per. 127d. Possible mass loss. Expanding circumstellar shell.
HR 526			BD+47 508	11031	37536				1438		01 49 15.7	+47 53 49	5.82	A3V	0.7	1.9	D:Component C 8.4v at 21", D 10.2v at 137".,SB:ADS 1438B.
HR 529			BD+51 416	11151	22678						01 50 57.1	+51 56 00	5.90	F5IV
HR 533		1	BD+54 396	11241	22690	2122				V436 Per	01 51 59.3	+55 08 51	5.52	B1.5V			G:In neutral hydrogen region; Cas-Tau OB1.,SB:15.6d, K 10k/s, V0 -9k/s.,VAR:E? 5.46 - 5.68y.
HR 536		2	BD+50 379	11291	22696	1052					01 52 09.4	+50 47 34	5.79	B9IIIpHgMn			SB:5.6270d, K 26.5k/s, V0 +11.4k/s, asini 2.05.
HR 538			BD+50 381	11335	22705						01 52 50.8	+51 28 29	6.26	A3V
HR 540			BD+54 408	11408	22716						01 53 48.5	+55 35 53	6.45	A5m
HR 568		3	BD+48 576	11949	37665						01 58 33.6	+49 12 15	5.69	K0IV
HR 590		4	BD+53 439	12303	22859	1054					02 02 18.1	+54 29 15	5.04	B8III
HR 618			BD+57 494	12953	22959					V472 Per	02 08 40.5	+58 25 25	5.67	A1Ia t			G:NGC 869; Per OB1.,S:Shell star.,VAR:Amp. 0.065V. Sp. var., H alpha profile var.
HR 621			BD+53 460	13137	22993	2146					02 10 07.8	+53 50 35	6.31	G8III
HR 627		5	BD+56 438	13267	23011				1685	Var?	02 11 29.0	+57 38 45	6.36	B5Ia	6.9	60.0	D:B, mag. diff 6.9v at 5.6".,G:Per OB1; h Per.
HR 641			BD+57 519	13476	23044						02 13 41.5	+58 33 40	6.44	A3Iab			G:Per OB1; h Per.
HR 654			BD+56 471	13854	23115			W		Var?	02 16 51.7	+57 03 19	6.48	B1Iab e	0.9	103.0	G:NGC 869 = h Per; Per OB1.
HR 661		8	BD+57 535	13982	23143	2157					02 17 59.9	+57 53 59	5.75	K3III
HR 662		7	BD+56 486	13994	23149				1753		02 18 04.5	+57 31 00	5.98	G7III	2.6	121.9	C:Heavily reddened.,G:May not be member of Per OB2.,N:Sometimes misidentified as Chi Per.
HR 685		9	BD+55 598	14489	23256	2159			1802	V474 Per	02 22 21.4	+55 50 44	5.17	A2Ia v	7.8	11.6	D:Fixed.,G:Per OB1.,RV:Var. in period over 200d.,S:Shell star.,VAR:Amp. 0.05V. Sp. and H alpha profile var.
HR 690			BD+54 535	14662	23283				1820	V440 Per	02 23 51.8	+55 21 52	6.28	F7Ib	8.1	10.0	VAR:CDelta, amp. 0.123V, 7.572d.
HR 696		10	BD+55 612	14818	23304					Var	02 25 16.0	+56 36 36	6.25	B2Ia e			G:Per OB1; in cluster Chi Per; NGC 884.,VAR:Amp. at 0.58 micrometers about 0.15m.
HR 716			BD+54 557	15253	23369				1878		02 29 25.0	+55 32 11	6.51	A2pShell v	1.3	2.8	D:Companion A3IV.,VAR:ADS 1878A, spectrum variable, shell star.
HR 785		11	BD+54 598	16727	23555	2188					02 43 02.8	+55 06 21	5.77	B7IIIpHg			SB:Double lines suspected.
HR 787			BD+52 616	16735	23556				2059		02 42 59.7	+53 31 34	5.84	K0II-III	9.0	12.4	D:Optical.
HR 788		12	BD+39 610	16739	55793	2187		S		896	02 42 14.9	+40 11 38	4.91	F9V	0.3	0.1	D:0.906y, a = 0.057".,DYN:0.046".,SB:331.0d, K 21.4k/s, V0 -21.5k/s, msin3i 0.744, asini 72.3. Speckle interferometer measurements combined with,SB:spectroscopic yield masses 1.28 and 1.05 solar. Speckle interferometric sep. 0.047", 1981.68.
HR 792			BD+47 683	16780	38274				2064		02 43 01.9	+48 15 56	6.48 R	G5II	5.0	72.8	D:AB fixed.,G:UMa stream.
HR 799	θ	13	BD+48 746	16895	38288	93	I		2081	902	02 44 12.0	+49 13 42	4.12	F8V	5.6	19.6	D:AB 4.13 F7V, 9.87 M1V, 2720y, a = 22.289". C probably optical.,DYN:0.095".
HR 800		14	BD+43 566	16901	38289	1077					02 44 05.2	+44 17 49	5.43	G0Ib-IICa1CH-1
HR 819			BD+35 553	17228	55868						02 46 58.3	+35 59 01	6.25	G8III			G:Probable Hyades group.
HR 820			BD+34 513	17240	55872				2117		02 47 03.5	+35 33 18	6.30 R	A9V	2.1	1.5	D:AB binary.
HR 825			BD+56 718	17378	23637			S		V480 Per	02 49 30.8	+57 05 03	6.25	A5Ia			G:Per OB1; vicinity of Perseus double cluster.,VAR:Amp. 0.038V.
HR 831			BD+36 566	17484	55910						02 49 27.1	+37 19 34	6.45	F6III-IV
HR 834	η	15	BD+55 714	17506	23655	99	I		2157		02 50 41.8	+55 53 44	3.76	K3-Ib-IIa e	4.7	28.3	C:Large infrared excess.,D:Component B, B9V, CPM, vsini 149k/s.,G:Red star Pleiades group.,N:Miram in Becvar; Allen says unnamed.,S:Ultraviolet FeII emission. Also classified K3Ib.
HR 840		16	BD+37 646	17584	55928	2194		W		956	02 50 35.1	+38 19 07	4.23	F2III	4.7	249.3	VAR:Delta Sct?
HR 842			BD+46 648	17656	38397	2197					02 51 41.7	+46 50 31	5.88	G8III
HR 843		17	BD+34 527	17709	55946	2198	I	A		963	02 51 30.8	+35 03 35	4.53	K5+III			S:Also classified K7III.
HR 846			BD+52 640	17743	23674				2185	971	02 52 52.0	+52 59 52	6.36	B8III	0.2	1.6	D:AB, 7.2, 9.2v sep. 0.2" possibly optical; AC binary.,DYN:0.006".
HR 849			BD+47 723	17818	38418				2192		02 53 21.2	+48 34 10	6.26	G5I	5.7	6.7
HR 854	τ	18	BD+52 641	17878	23685	103	I		2202	Tau Per	02 54 15.5	+52 45 45	3.95	G4III+A4V	8.6	51.7	D:A* 4.06 G4III+A4V, 4.150y, a = 0.050". Speckle interferometric sep. 0.080" 1981.67. Circumstellar material surrounding,D:the pair? Visual companions 10.7v at 51" possibly physical; 11.8v at 4" possibly optical.,SB:ADS 2202A, 1515.6d, K 19.0k/s, V0 +2.2k/s, asini 271. vsini of secondary 50k/s.,VAR:EA, 3.94 - 4.07V.
HR 855		20	BD+37 655	17904	55975				2200	977	02 53 42.6	+38 20 15	5.33	F4IV	0.6	0.2	D:AB 5.9 F4V, 6.5 F6V, 31.37y, a = 0.258". Nearly equal components, 3.7, 4.3 solar. Component C, 9.7v at 14", CPM?,DYN:0.013".,SB:ADS 2200A, 1269d, K 4.8k/s, V0 +2.4k/s, asini 73.0. Orbit questioned by Morbey and Griffin (1987, ApJ, 317,,SB:343). Resolved by speckle interferometry 1983.93, sep. 0.20"; 1983.94, sep. 0.18".,VAR:Delta Sct?
HR 864			BD+50 665	18153	23721						02 56 50.6	+51 15 39	6.22	K5III
HR 865			BD+46 658	18155	38455			W			02 56 33.4	+47 09 50	6.02	gK3	5.5	24.9	D:Component B, 15v, possibly spurious.
HR 873		21	BD+31 509	18296	56031	2205				LT Per	02 57 17.3	+31 56 03	5.11	B9pSi v			G:Member moving cluster in Perseus.,S:Underabundance of magnesium and oxygen.,SB:2.88d.,VAR:Alpha CV 5.03 - 5.14V, 2.88422d, same for RV and line-intensities. Also var. magnetic field and H-lines. Rotating,VAR:spotted star.
HR 876			BD+38 599	18339	56036		I				02 58 02.3	+38 36 54	6.04	gK3
HR 879	π	22	BD+39 681	18411	56047	2207					02 58 45.7	+39 39 46	4.70	A2Vn			N:Gorgonea Secunda.
HR 882		24	BD+34 550	18449	56052	1082	I				02 59 03.7	+35 10 59	4.93	K2III
HR 885			BD+46 669	18474	38493						02 59 49.9	+47 13 15	5.47	G5:III*			S:G5:III: CN-4 CH-1 Ca 1 H delta-1. Also classified G8III CH weak. Noted as having composite spectrum, but unresolved,S:by speckle interferometry 1981.69.
HR 886			BD+40 639	18482	38492		I			1004	02 59 39.9	+41 01 59	5.89	K2
HR 890			BD+51 665	18537	23763				2270 A		03 00 52.2	+52 21 06	5.28	B7V	1.4	11.9	D:CPM with HR 891.,G:Per OB3.
HR 891			BD+51 665	18538	23765				2270 B		03 00 53.4	+52 21 08	6.74	B9V	1.4	11.9	D:CPM with HR 890.,G:Per OB1?
HR 894			BD+37 675	18552	56067						03 00 11.8	+38 07 54	6.11	B8Vne			S:Shell star. Near IR spectroscopy indicates presence of cool companion.
HR 915	γ	23	BD+52 654	18925	23789	108	I		2324		03 04 47.8	+53 30 23	2.93	G8III+A2V	8.6	57.0	D:SKYLAB observations indicate cool star with hot companion. Components Aa, 14.65y, a = 0.159". Physical nature of B,,D:11m at 57", uncertain.,M:Close to error box of X-ray source 3U0305+53.,SB:5350d, K 12.7 or 21.9k/s, V0 +2.5k/s, msin3i 4.87, asini 648. vsini of secondary 50k/s. Resolved by speckle,SB:interferometry 1981.67, sep. 0.284", 1983.93, sep. 0.27".
HR 918			BD+56 767	18970	23791	2217	I				03 05 32.4	+56 42 21	4.76	G9.5III
HR 920			BD+55 738	18991	23793						03 05 39.9	+56 04 07	6.11	G9III
HR 921	ρ	25	BD+38 630	19058	56138	109	I			Rho Per	03 05 10.6	+38 50 25	3.39	M4II			G:Zeta Her group.,N:Gorgonea Tertia.,VAR:SRb 3.30 - 4.0V, about 50d with possibly slow var. in mean brightness in 1100d period.
HR 923			BD+40 664	19066	38559						03 05 20.8	+40 34 57	6.05	K0III
HR 930			BD+51 681	19268	23825						03 08 03.9	+52 12 48	6.31	B5V
HR 933			BD+46 692	19279	38587						03 07 47.4	+47 18 30	6.41	A3Vnn
HR 936	β	26	BD+40 673	19356	38592	111	I		2362	Bet Per	03 08 10.1	+40 57 20	2.12	B8V	8.3	81.9	C:Color excess E(B-V) = +0.03.,D:A* var. B8V, 1.858y, a = 0.011" or 1.862y, a = 0.104". Apparent apsidal period 28.4y or 32y. Resolved by speckle,D:interferometry: sep. 0.086", 2-3v fainter than primary. This may be Algol C. Four visual companions all optical:,D:B, 12.7v at 59"; C, 12.5 at 67"; D, 10.5 at 82"; BC sep. 15"; E, 12.5v at 11" from D.,M:One of the few known galactic radio sources in which the dominant star is normal. 21cm radio source.,N:ALGOL; Gorgona; Gorgonea Prima; Demon Star; El Ghoul.,S:B8V+G.,SB:Algol ABxC: 1.8613y, K 12.0k/s, V0 +3.7k/s, msin3i 3.91, asini 109. Spectra B8V, G5IV, Am. Mass Algol AB, 5.3,SB:Suns; C, 1.8 Suns. Circumstellar gas fills Roche lobe of hot component. ADS 19356A: 2.8673d, K 44.0k/s, V0 var.,,SB:asini 1.73. Resolved by speckle interferometry 1982.17, sep. 0.052", 1983.94, sep. 0.08".,VAR:ADS 2362A is the prototype Algol star, first discovered as variable by Montanari in 1669. The first period determined by,VAR:Goodricke in 1783, who also interpreted the variations as due to eclipses. The prototype star proves to be a more,VAR:a complicated system than most of the Algol-type stars, i.e., compact triple system with separation of the components,VAR:well under 0.1". The components usually designated Algol A, B, C, sometimes A, a, P. Two formerly additionally desig-,VAR:nated components D and E, inferred on the basis of an apparent 32 year apsidal motion, are now considered spurious.,VAR:The various Algol components must not be confused with the visual components ADS 2362 B-E, optical companions at much,VAR:greater distances from A. ADS 2362A, EA 2.12 - 3.40V, 2.86732442d, abrupt period changes. Orbital and rotation periods,VAR:synchronized. Rotational velocity 65k/s. Radio flares extending to about 1 A.U., not associated with X-ray activity.,VAR:Radio flare activity appears correlated with period discontinuities, attributed to "starquakes." Mass flow from K to B8,VAR:component at rate of 1.8x10E-08 solar masses/year. Possible circumstellar material associated with radio or H alpha,VAR:emission.
HR 937	ι		BD+49 857	19373	38597	112	I	W			03 09 04.0	+49 36 48	4.05	G0V	8.2	146.2	G:Mel 20 #44, but not cluster member; Per OB3.
HR 941	κ	27	BD+44 631	19476	38609		I		2368	1055	03 09 29.8	+44 51 26	3.80	K0III	8.4	27.7	D:Companion optical.,G:Hyades group.
HR 947	ω	28	BD+39 724	19656	56224		I	W			03 11 17.4	+39 36 42	4.63	K1III	6.1	177.4	N:Gorgonea Quarta.
HR 949			BD+47 779	19735	38638	2225	I	W			03 12 26.4	+47 43 33	6.33	K5III	3.9	202.1	G:Mel 20 #138; Per OB3.
HR 950			BD+41 631	19736	38635						03 12 09.6	+42 22 34	6.15	B4V			G:Member of the local association (Pleiades group).
HR 956			BD+47 782	19845	38652						03 13 24.0	+48 10 37	5.90	G9III			G:Mel 20 #175; Per OB3. Nonmember of Alpha Per cluster on basis of RV.,M:Space motion same as for Hyades cluster.
HR 964			BD+56 798	20041	23903				2424		03 15 48.0	+57 08 27	5.79	A0Ia	8.2	10.8	G:In reflection nebula; member assoc. Cam R1 at about 870 pc. Cam OB1.
HR 966			BD+41 638	20063	38674						03 14 56.7	+42 30 14	6.07 R	K2III			S:Strong CN.
HR 969			BD+50 729	20123	23914		I				03 16 12.2	+50 56 16	5.03	G6Ib-IIa			G:Mel 20 #308; Per OB3.,SB:5.543491d.
HR 973			BD+44 648	20162	38685		I				03 16 04.7	+45 20 45	6.16	M2III
HR 975			BD+32 591	20193	56293				2431		03 15 47.0	+32 51 23	6.31	F4V vw	6.5	44.1
HR 976			BD+34 610	20210	56296				2433	V423 Per	03 16 01.9	+34 41 19	6.25	A1m	7.2	29.3	SB:ADS 2433A, 5.5435d, K 62.7k/s, V0 +24.2k/s, asini 4.78.,VAR:Ell 6.16 - 6.28V, 5.543491d.
HR 978			BD+31 576	20277	56308						03 16 35.1	+32 11 01	6.06	G8IV
HR 979			BD+39 743	20283	38700				2443		03 17 11.4	+40 29 00	6.45	B9VpSi	0.9	3.8	D:Component B, 8.0 A7m. CPM.
HR 982		30	BD+43 674	20315	38704						03 17 47.4	+44 01 30	5.47	B8V			G:Per OB3; nonmember of Alpha Per cluster on basis of RV.
HR 986			BD+38 690	20346	56322	2230					03 17 45.8	+39 17 00	5.96	A2IV
HR 987		29	BD+49 899	20365	23944						03 18 37.8	+50 13 20	5.15	B3V			G:Per OB3.,SB:1.996933d.
HR 989		31	BD+49 902	20418	38714						03 19 07.6	+50 05 42	5.03	B5V			G:Per OB3.
HR 991			BD+33 619	20468	56340	2232	I				03 18 43.8	+34 13 22	4.82	K2IICN1			S:Also classified K2III CN2 Ba 0.3.
HR 1001			BD+48 893	20675	38753			W			03 21 52.6	+49 04 15	5.93	F6V	3.5	205.8	G:Hyades moving group; Per OB3; Mel 20 #497.
HR 1002		32	BD+42 750	20677	38750	2236				1107	03 21 26.5	+43 19 46	4.95	A3V
HR 1011			BD+48 899	20809	38768						03 23 13.2	+49 12 48	5.29	B5V			G:Mel 20 #557; Per OB3; nebulosity.,SB:Possibly long period.
HR 1017	α	33	BD+49 917	20902	38787	120	I	W		1125	03 24 19.4	+49 51 40	1.79	F5Ib	10.0	167.0	G:Mel 20 #605; Per OB3; nebulosity.,N:MIRPHAK; Mirfak; Marfak; Algenib.
HR 1019			BD+33 636	20995	56419				2514		03 24 29.7	+33 32 09	5.61 R	A0V	3.5	4.3	D:AB CPM.
HR 1020			BD+53 657	21004	24024						03 25 48.4	+53 55 18	6.51	A9III-IV
HR 1026			BD+40 736	21038	38809						03 25 09.4	+41 15 26	6.51	A0V
HR 1029			BD+48 913	21071	38817						03 25 57.4	+49 07 15	6.09	B7V			G:Mel 20 #675; Per OB3.
HR 1034			BD+48 920	21278	38849						03 28 03.1	+49 03 46	4.98	B5V			C:Color excess E(B-V) = +0.10.,G:Mel 20 #774; Per OB3.,S:Lyman alpha observed from COPERNICUS.,SB:21.659d, K 25.0, V0 -0.5, asini 7.34.
HR 1037			BD+49 944	21362	38862						03 28 52.4	+49 50 54	5.58	B6Vn			G:Mel 20 #810; Per OB3.
HR 1041			BD+33 656	21402	56475						03 28 20.8	+33 48 27	5.61 R	A2V
HR 1044		34	BD+49 945	21428	38872				2558		03 29 22.1	+49 30 32	4.67	B3V	2.1	0.8	D:550y.,G:Mel 20 #835; Per OB3.
HR 1047			BD+46 760	21455	38874				2560		03 29 26.2	+46 56 16	6.24	B7V	5.1	27.9	G:Mel 20 #861; Per OB3. Nonmember of Alpha Per cluster on basis of RV.
HR 1051			BD+47 844	21551	38893						03 30 37.0	+48 06 13	5.82	B8V			G:Mel 20 #904; Per OB3.,S:Shell star.
HR 1052	σ	35	BD+47 843	21552	38890	124	I			1167	03 30 34.5	+47 59 43	4.36	K3III			G:Mel 20 #900; Per OB3.
HR 1056			BD+48 938	21620	38906					1173	03 31 29.4	+49 12 35	6.29	A0Vn			G:Mel 20 #934; Per OB3.,VAR:EA, amp. 0.1V, 5.363d.
HR 1059			BD+48 942	21661	38912						03 31 49.1	+49 24 03	6.39	B9III			G:Mel 20 #954; Per OB3.
HR 1063			BD+47 847	21699	38917					V396 Per	03 32 08.6	+48 01 25	5.47	B8IIIpMn			G:Mel 20 #985; Per OB3.,S:Spectra show Mn. Helium weak. Si enhanced. Also classified B5Vp.,VAR:Alpha CV 5.45 - 5.53V, 2.4928d. First helium-weak star found to have periodic variations (1973).
HR 1069		36	BD+45 778	21770	38924	2249				1182	03 32 26.3	+46 03 25	5.31	F4III
HR 1072			BD+44 734	21803	38927					KP Per	03 32 39.1	+44 51 20	6.41	B2IV			G:Cas-Tau OB1.,VAR:Beta C 6.37 - 6.47V, 0.2101753d, multiple periods, 0.1982, 10.85, 0.01d.
HR 1074			BD+34 674	21856	56531	1098				Var?	03 32 40.0	+35 27 42	5.90	B1V			G:Per OB2.
HR 1078			BD+39 811	21912	56538	2254				IW Per	03 33 35.1	+39 53 58	5.81	A5m			SB:0.9171877d, K 99.3k/s, V0 +0.2k/s, asini 1.251.,VAR:Ell 5.80 - 5.85V, 0.9171877d.
HR 1087	ψ	37	BD+47 857	22192	38980		I			Psi Per	03 36 29.4	+48 11 34	4.23	B5Ve v			G:Mel 20 #1164; Per OB3; member of Pleiades group. Nonmember of Alpha Per cluster on basis of RV.,RV:Rotationally unstable shell star.,S:Shell star.,VAR:Amp. 0.04V, 0.5d. Hydrogen emission variable. Expanding circumstellar shell.
HR 1097			BD+42 795	22402	38999						03 38 00.2	+42 34 59	6.42	B8Vn
HR 1113			BD+37 811	22780	56628					1225	03 41 07.9	+37 34 48	5.57	B7Vne			G:Member of the local association (Pleiades group).,VAR:Gamma Cas?, 5.55 - 5.58V.
HR 1122	δ	39	BD+47 876	22928	39053	131		W		Del Per	03 42 55.5	+47 47 15	3.01	B5IIIe t	7.3	99.1	C:Color excess E(B-V) = +0.04.,G:Per OB3.,S:C1 neutral carbon continuum shows discontinuities in UV. Lyman alpha observed from COPERNICUS.,VAR:Alpha CV? 2.98 - 3.03V, about 1d. Strong variable emission at 1650A, CaII?
HR 1123		40	BD+33 698	22951	56646				2699		03 42 22.5	+33 57 54	4.97	B0.5V	5.0	20.0	C:Reddened star. Color excess E(B-V) = +0.24.,G:Per OB2.
HR 1127			BD+48 984	23049	39063		I		2712		03 44 06.4	+48 31 25	6.06	K4III	7.1	18.6	C:Nicolet has 6.60V, Mermilliod 6.39V: no indication of variability.
HR 1130			BD+45 804	23139	39071	2266					03 44 40.9	+46 05 59	6.11	A7IV
HR 1131	ο	38	BD+31 642	23180	56673				2726	Omi Per	03 44 19.1	+32 17 18	3.83	B1III	2.8	1.0	C:Reddened star. Color excess E(B-V) = +0.32.,D:Binary. Combined mag., colors. Rotational velocity B, 150:k/s. Unresolved by speckle interferometry 1982.16.,DYN:0.005".,G:Per OB2 (not a member). Embedded in reflection nebulosity. In cluster IC 348.,M:In interstellar ultraviolet radiation field.,N:Atik; Ati; Al Atik.,P:Intrinsic polarization, probably due to circumstellar matter.,SB:4.4192d, K 109.3k/s, V0 +19.8k/s, msin3i 5.26, asini 6.63. Rotational velocity of secondary, 84k/s, primary,SB:85k/s.,VAR:Ell 3.79 - 3.85V, 4.419171d, possibly half.
HR 1133			BD+36 742	23193	56675	2268					03 44 31.4	+36 27 36	5.59	A2m
HR 1135	ν	41	BD+42 815	23230	39078	134	I		2738	1261	03 45 11.6	+42 34 43	3.77	F5II	8.1	31.4
HR 1141			BD+45 811	23300	39085				2746		03 45 59.3	+45 40 55	5.66	B6V	8.4	6.5	D:CPM.,G:Member of the local association (Pleiades group).
HR 1160			BD+50 825	23552	24231				2769		03 48 18.3	+50 44 12	6.14	B8Vne	6.2	7.0	D:Probably optical.,S:Shell star.
HR 1163			BD+33 717	23625	56709				2772	1305	03 47 52.6	+33 36 00	6.57	B2.5V	4.0	3.2	D:Binary.,G:Per OB2.,SB:ADS 2772A, 1.9406d, K 82k/s, V0 +20k/s, msin3i 0.883, asini 2.19.,VAR:B-A varies from 2.8 to 4.3V. Uncertain which component varies.
HR 1164			BD+31 650	23626	56707						03 47 48.9	+32 11 42	6.25	G0
HR 1170			BD+43 818	23728	39128					V376 Per	03 49 08.2	+43 57 47	6.02	A9IV			VAR:Delta Sct 5.8 - 5.91V, variable amp. Primary and beat periods, 0.098299 and 0.39206d.
HR 1176			BD+44 801	23838	39134					Var?	03 50 04.5	+44 58 04	5.66	G2III+F2:V			SB:vsini of secondary 85k/s. Unresolved by speckle interferometry 1983.93.,VAR:A variable comparison star was used when HR 1176 was suspected of variablility.
HR 1177		42	BD+32 667	23848	56727					V467 Per	03 49 32.6	+33 05 29	5.11	A3V			G:Per OB2.,SB:1.7653d, K 34.4k/s, V0 -11.9k/s, asini 0.832.,VAR:A published period, 22.58d, does not satisfy available SB observations, whereas the SB period does satisfy the,VAR:photometric equally well. However, more observations are badly needed.
HR 1191			BD+33 728	24131	56761			W			03 51 53.7	+34 21 33	5.77	B1V	7.5	15.1	G:Per OB2.
HR 1197			BD+30 582	24167	56762						03 52 04.3	+31 10 06	6.25	A5V			G:Per OB2.
HR 1198			BD+48 1015	24240	39175						03 53 38.7	+48 39 02	5.76	K0III
HR 1203	ζ	44	BD+31 666	24398	56799	144	I		2843	1397	03 54 07.9	+31 53 01	2.85	B1Ib	6.5	12.9	C:Reddened star. Color excess E(B-V) = +0.33.,D:AB CPM, B 9.16V B8IV; C, 9.12V at 33" optical; D, 10.35V, +0.713(B-V), +0.20(U-B), at 92" optical; E, 9.90V, A2V,,D:+0.33(B-V), +0.17(U-B), at 120" physical.,DYN:0.012".,G:IC 348; Per OB2.,RV:Comp. B +20.8k/s.,S:Interstellar CH detected optically. COPERNICUS data used to analyze the chemical abundances in line of sight to,S:Zeta Per: CO, HD, and OH. About 60% of the hydrogen in front of the star is molecular.,SB:1.765d, K 6.0k/s, V0 +22.2k/s.,VAR:2.80 - 2.93V.
HR 1207			BD+47 912	24504	39195	2279					03 55 58.2	+47 52 17	5.37	B6V			G:Per OB3.
HR 1209			BD+30 591	24534	56815		I		2859	X Per	03 55 23.0	+31 02 45	6.10	O9.5ep v	5.8	22.5	C:Heavily reddened.,D:CPM? Component A possibly optical counterpart or companion of X-ray source 4U0352+30. Possibly a triple system with a,D:neutron star moving around the optical primary in 22.4 hrs., and either apsidal period 581d or close double moving,D:around a distant component in 581d. Rotational velocity of primary, vsini 306k/s. Component ADS 2859B is normal M1III,,D:not T Tau type as once assumed.,G:May not be member of Per OB2; Zeta Per group.,M:Space velocities of X Per and Xi Per indicate the two stars approached to within 17 pc 2 million yrs ago.,P:Conflicting evidence whether observed polarization is intrinsic to the star or of interstellar origin.,S:Sp. data suggest occasional interruption of almost steady infall of material through rotating emission region by,S:outbursts of material from the star.,SB:580.7d, K 59k/s, V0 -50k/s, asini 471. Emission lines var. in RV, 22.4 hrs. and 581d.,VAR:ADS 2859A, Gamma Cas 6.07 - 7.0V, 580.7?d. Amp. about 0.02U. X-ray period 22.4 hrs. Spectrum variable. Sudden,VAR:decrease in H alpha emission followed by 450 sec. flare in continuum. Possible neutron star companion pulsating in,VAR:13.924 min. Simultaneous X-ray and optical obs. 21 Jan. 1975 showed X-ray var. by factor 2 but no corresponding optical,VAR:100 sec. quasi periodic photometric var. may indicate binary with compact companion undergoing mass accretion.
HR 1210		43	BD+50 860	24546	24314		I	W			03 56 36.5	+50 41 43	5.28	F5IV	4.8	75.3	C:IR source in this direction corresponds to a Seyfert galaxy.,D:AB CPM. Component C, 11.4v at 101" optical. P, 12.5v at 279".,G:Hyades moving group.,SB:30.4380d, K 51.9k/s, V0 +25.1k/s, msin3i 0.910, asini 16.9; alternate orbit 30.4391d, K50.6k/s,,SB:msin3i 0.82, asini 15.53; vsini both components <17k/s.
HR 1215			BD+34 768	24640	56824					1418	03 56 28.7	+35 04 52	5.49	B1.5V			G:Per OB2.,VAR:Beta C?, 5.45 - 5.50V. RV possibly var. 0.13169d.
HR 1220	ε	45	BD+39 895	24760	56840	147			2888	Eps Per	03 57 51.2	+40 00 37	2.89	B0.5V+A2V	5.1	8.8	C:Color excess E(B-V) = +0.10.,D:AB CPM. B, 7.39V, -0.03(B-V), -0.52(U-B), B9.5V, vsini 300:k/s.,G:Cas-Tau OB1; member of Pleiades group.,VAR:Beta C, 2.88 - 3.00V, 0.216:d. Brightest component on visual triple. Photoelectric and spectroscopic resonant periods,VAR:found are submultiples of 26.9 hrs or 1.12d.
HR 1223			BD+34 773	24809	56847					V386 Per	03 58 03.1	+34 48 52	6.53	A8V			G:Per OB2.,SB:vsini both components 80k/s.,VAR:Delta Sct 6.50 - 6.58V, 0.052d.
HR 1226			BD+38 827	24843	56849						03 58 29.1	+38 50 25	6.30	gK1
HR 1228	ξ	46	BD+35 775	24912	56856	148	I			Xi Per	03 58 57.9	+35 47 28	4.04	O7.5III(n)((f)) e			C:Color excess E(B-V) = +0.32.,G:Runaway star from Per OB2. Within 1d and exciting star of HII region S220. Ionizes region at edge of California nebula =,G:NGC 1499.,N:Menkib; Menkhib; Menchib.,S:Interstellar CO emission. Central Balmer emission in blue-violet only.,SB:6.951d.,VAR:Slightly variable, possibly same period as SB.
HR 1229			BD+38 829	24982	56866				2910		03 59 40.0	+38 49 14	6.38 R	A1Vp:	2.7	1.5
HR 1234			BD+36 805	25152	56899						04 01 14.7	+36 59 24	6.41	A0V			RV:Determinations of vsini range from 50 to 250k/s.
HR 1261	λ	47	BD+49 1101	25642	24412	1113					04 06 35.0	+50 21 05	4.29	A0IVn
HR 1273		48	BD+47 939	25940	39336	152	I			MX Per	04 08 39.7	+47 42 45	4.04	B3Ve			G:Per OB3; member of Pleiades group.,RV:Pole on.,S:Excess IR emission.,SB:16.934615d not confirmed.,VAR:Gamma Cas 4.00 - 4.10V, 55?d. Slow var. possibly associated with emission spectrum.
HR 1277		49	BD+37 881	25975	57000						04 08 15.3	+37 43 40	6.09	K1III
HR 1278		50	BD+37 882	25998	57006	2297					04 08 36.6	+38 02 23	5.51	F7V			D:CPM with GC 4949 at 12' = ADS 2995, a triple system 7.3 dK2, 9.0 sep. 1"; C at 234".,G:Hyades group.
HR 1286			BD+33 807	26311	57047	2300	I				04 10 59.0	+33 35 12	5.72	K1II-III
HR 1301			BD+37 897	26605	57081						04 13 59.6	+37 58 01	6.45 R	G9III
HR 1303	μ	51	BD+48 1063	26630	39404	1117	I		3071	1518	04 14 53.9	+48 24 34	4.14	G0Ib	6.0	83.8	D:A* 4.13 G0Ib, 0.778y, a = 0.019". AB CPM; B, 11.8v at 15". C , 10.25V, +0.47(B-V), +0.06(U-B), B8.,SB:283.272d, K 20.7k/s, V0 +7.7k/s, asini 80.5. Unresolved by speckle interferometry.,VAR:ADS 3071A, 4.1 - 4.24V.
HR 1306		52	BD+40 912	26673	39409	2306	I				04 14 53.3	+40 29 01	4.71	G5Ib+A2V			SB:1576.44d, K 18.1k/s, V0 -4.5k/s, asini 358. Unresolved by speckle interferometry 1983.93. vsini of secondary,SB:100k/s.
HR 1324			BD+49 1150	26961	24531					b Per	04 18 14.6	+50 17 44	4.61	A2V			G:In NGC 1545 #1; Hyades group.,M:Source of weak radio emission.,SB:Comp. ABC: 701.76d, K 11.4k/s, V0 +21k/s, asini 107. Comp. A: 1.527365d, K 39.4k/s, V0 var., asini 0.827.,SB:Unresolved by speckle interferometry.,VAR:Ell 4.59 - 4.65V, 1.527365d. Radio binary showing radio flare activity. Third component may eclipse primary.
HR 1328			BD+41 844	27026	39447						04 18 08.2	+42 08 28	6.22	B9V
HR 1330			BD+49 1155	27084	39457						04 19 13.3	+50 02 56	5.45	A7V			G:NGC 1545 #1.
HR 1333			BD+50 973	27192	24544	2316				1550	04 20 11.5	+50 55 15	5.55	B1.5IV			G:Cas-Tau OB1.,SB:1.527365d, K 38.83k/s, V0 +20.66k/s, asini 0.815.,VAR:Amp. 0.020V.
HR 1337			BD+41 852	27278	39468						04 20 14.4	+41 48 29	5.92	K0III
HR 1343		54	BD+34 860	27348	57171	158	I	W			04 20 24.6	+34 34 00	4.93	G8III	7.9	110.0
HR 1344			BD+31 757	27349	57166		I				04 20 10.0	+31 57 12	6.16	K5
HR 1350		53	BD+46 872	27396	39483	2319				V469 Per	04 21 33.2	+46 29 56	4.85	B4IV			G:Member of Pleiades group.,SB:Same period as VAR.,VAR:Amp. 0.01V, 7.29?hrs.
HR 1371			BD+42 946	27650	39501				3172		04 23 35.9	+42 25 41	6.23	A1pSi	0.5	0.4
HR 1377		55	BD+33 853	27777	57212						04 24 29.2	+34 07 50	5.73	B8V
HR 1379		56	BD+33 854	27786	57216				3188	1592	04 24 37.4	+33 57 35	5.76	F4V	3.6	4.9	DYN:0.042".,VAR:ADS 3188B, 9.6 - 11.3v.
HR 1390			BD+31 776	27971	57229	2325					04 26 06.3	+31 26 20	5.28	K1III
HR 1419			BD+32 806	28459	57269			W			04 30 38.3	+32 27 29	6.21	B9.5Vn			D:Suspected of being double; probably single.
HR 1424			BD+39 1013	28503	57278				3273 A		04 31 24.0	+40 00 37	6.26	B8V	0.5	9.3	D:CPM.
HR 1434		57	BD+42 990	28704	39604	1124		W			04 33 24.9	+43 03 50	6.09	F0V	0.7	116.2
HR 1454		58	BD+40 1000	29094	39639	2338	I	A			04 36 41.4	+41 15 53	4.25	K4III+A3V		0.1	D:A* 4.27 G8II+B, 28.67y, a = 0.054"(not confirmed).,S:Also classified K0II-III + B9V.,SB:10,470d, K 12.8k/s, V0 +5.9k/s, asini 1400. One of the longest SB periods known, 28.67y. Masses 6 and 5 solar.,SB:Unresolved by speckle interferometry. vsini of both components =<50k/s.
HR 1482			BD+48 1128	29526	39688	2347					04 41 24.1	+48 18 03	5.67	A0V
HR 1489			BD+37 954	29645	57377	2348					04 41 50.3	+38 16 49	5.99	G0V
HR 1493			BD+49 1230	29721	39702	1128		W			04 43 21.6	+49 58 26	5.87	B9III	7.3	20.8
HR 1494		59	BD+43 1043	29722	39699	2349					04 42 54.3	+43 21 54	5.29	A1Vn
HR 1500			BD+40 1032	29866	39715						04 44 12.9	+40 47 13	6.08	B8IVne			S:Shell star.
HR 1514			BD+40 1045	30138	39746						04 46 44.4	+40 18 46	5.97	G9III
HR 1533			BD+37 969	30504	57447	1133	I				04 49 54.6	+37 29 18	4.88	K3.5IIIBa0.2:			N:Formerly 1 Aur, now in Perseus.

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

Perseus / Yale Bright Star Catalog (HR)

Legend

References