Catalogues

Catalogue

Constellation

Aries / 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 522		4	BD+16 203	10982	92637	1050					01 48 10.9	+16 57 20	5.84	B9.5V
HR 530		1	BD+21 243	11154	74966				1457		01 50 08.5	+22 16 31	5.86	K1III+A6V	1.1	2.8	D:Binary. Component B 7.3v A6V, P.A. 166d; RV, 1.8k/s, variable. Confusion in literature as to which component is HD,D:11154, which 11155. Probably combined mag. and color.,DYN:0.006".,G:UMa stream.
HR 534			BD+10 252	11257	92659			D		635	01 50 52.0	+11 02 36	5.94	F2V w	0.0	0.1	G:UMa stream.,N:54 Cet in Aries.
HR 545	γ¹	5	BD+18 243	11503	92680				1507 B	Var?	01 53 31.8	+19 17 45	4.83 H	B9V v	0.1	7.8	D:Binary with HR 546, q.v. Combined mag. HR 545/6, 3.88V; colors also combined.,DYN:0.019".,N:The HD numbers and other data, especially spectral classes, for HR 545-6 have frequently been interchanged. HD 11502 is,N:the brighter = HR 546, while HD 11503 = HR 545 is the slightly fainter N. prec. component B of ADS 1507.,VAR:Sp. var. 38 min.
HR 546	γ²	5	BD+18 243	11502	92681				1507 A	Gam Ari	01 53 31.8	+19 17 37	4.75 H	A1pSi	0.1	7.8	D:Binary with HR 545, orbital period 5000 - 10000y? Component C, 9.6v at 221". Combined colors for HR 545-6; combined,D:mag. 3.88V.,DYN:0.019".,G:Pleiades group.,N:Mesarthim; Mesartim; "First Star in Aries".,S:Also classified A0pCr, A1pCrSiSr.,VAR:Alpha CV 3.88 - 3.90V, 2.6095 or 1.7982d; also possibly 2.5 hrs., amp. 0.02, unconfirmed. Southern component of,VAR:ADS 1507. Magnetic var.
HR 553	β	6	BD+20 306	11636	75012	66	I			658	01 54 38.4	+20 48 29	2.64	A5V			N:Sharatan; Sheratan; Al Sharatain.,SB:106.9973d, K 37.1k/s, V0 -4.0k/s, asini 23.8. One of the most eccentric orbits known: e 0.892. Binary unresolved by,SB:speckle interferometry 1981.69. SB2 in infrared: near-IR reticon spectra at 8800 Ang show double lines and indicate,SB:that the secondary is late F- or G-type main-sequence star.,VAR:Delta Sct?
HR 559		7	BD+22 284	11763	75030	2130	I			RR Ari	01 55 51.0	+23 34 38	5.74	K1III			VAR:EA? 6.42 - 6.84p, 47.9?d.
HR 563	ι	8	BD+17 289	11909	92721	2132	I				01 57 21.1	+17 49 03	5.10	K1p	1.0	0.0	S:Also classified G2Ib-II.,SB:1567.66d, K 10.8k/s, V0 -4.9k/s, asini 217, 5.4, 6.4v, sep. 0.01", unresolved by speckle interferometry.
HR 569	λ	9	BD+22 288	11973	75051				1563 A	680	01 57 55.7	+23 35 46	4.79	F0V	2.5	37.4	D:ADS 1563B, 7.40V, +0.58(B-V), +0.07(U-B), dG1, CPM; vsini =<25k/s.,VAR:ADS 1563B; Cst? 7.30 - 740V.
HR 577			BD+20 322	12139	75077				1582 D		01 59 35.7	+21 03 30	5.87	K0III-IV	3.3	188.1	D:ADS 1582AB, 8.5, 11.0v, sep. 2.3" at 188" from the bright component D. C, 9.2v at 31" from A.
HR 578			BD+11 261	12140	92739	2136					01 59 25.9	+12 17 41	6.09	A6V
HR 601			BD+12 271	12479	92763		I				02 02 35.2	+13 28 36	5.94	M2III			R:Occultation diam., two determinations, 0.0026" and 0.0036".
HR 605		10	BD+25 341	12558	75114				1631		02 03 39.3	+25 56 08	5.63	F8IV	1.5	0.8	D:AB 5.90 F8IV, 7.27 F9V, 288.0y, a = 1.256"; or 309.03y, a = 1.34". Other published periods have ranged from 247 to,D:925y. Combined mag., colors.,DYN:0.016".
HR 609			BD+17 307	12594	92774		I	D			02 03 42.6	+18 15 12	6.21	gK4			D:Suspected occultation double.
HR 613	κ	12	BD+21 279	12869	75146						02 06 33.9	+22 38 54	5.03	A2m			SB:15.2938d, K 34.4k/s, V0 +11.5k/s, msin3i 0.137, asini 5.75.
HR 615		11	BD+25 349	12885	75149				1658		02 06 49.2	+25 42 17	6.15	B9IV-Vn	5.5	1.6
HR 617	α	13	BD+22 306	12929	75151	74	I			725	02 07 10.4	+23 27 45	2.00	K2-IIICa-1			N:HAMAL; Hemal; Hamul; Ras Hammel; El Nath (obsolete). The name Arietis also used both for the star and the constellation.,S:Also classified K2IIIab Ca-1.
HR 623		14	BD+25 355	13174	75171			W			02 09 25.3	+25 56 23	4.98	F2III	2.5	105.9
HR 624			BD+16 247	13201	92810						02 09 23.1	+17 13 28	6.43	F5V
HR 631		15	BD+18 277	13325	92822	1056	I			738	02 10 37.6	+19 30 01	5.70	M3IIIab
HR 633		16	BD+25 362	13363	75188		I				02 11 12.0	+25 56 13	6.02	gK4
HR 644			BD+23 297	13522	75203		I				02 12 37.5	+24 10 04	5.96	K0
HR 646	η	17	BD+20 348	13555	75204						02 12 48.1	+21 12 39	5.27	F5V			M:Possible nearby star on basis of spectroscopic parallax.
HR 648		19	BD+14 357	13596	92841	1057	I			748	02 13 03.3	+15 16 47	5.71	M0III			G:Zeta Her group.
HR 656		20	BD+25 373	13871	75239						02 15 46.0	+25 46 59	5.79	F6IV-V			G:Hyades group; Mel 25 #157.
HR 657		21	BD+24 329	13872	75238	1059		W			02 15 42.8	+25 02 35	5.58	F6V	0.3	0.2	D:19.35y, a 0.17" or 18.614y, e 0.616, a 0.158", 10.82AU, i 130.1d. Alternate orbit 19.35y, a = 0.17". Speckle,D:interferometric sep. 0.17", 1983.93.,M:Possible nearby star on basis of spectroscopic parallax.
HR 665			BD+23 307	14067	75262	2156					02 17 10.4	+23 46 04	6.55	G9III
HR 669	θ	22	BD+19 340	14191	92877	81					02 18 07.5	+19 54 04	5.62	A1Vn
HR 676			BD+22 329	14262	75277						02 18 58.0	+23 10 04	6.46	A1V+F3III			SB:363.51d, K 19.4k/s, V0 -24.64k/s, asini 91.5; vsini of secondary 110k/s.
HR 702	ξ	24	BD+09 316	14951	92932	2164					02 24 49.0	+10 36 38	5.47	B7IV
HR 711			BD+26 409	15152	75370		I				02 27 07.0	+27 00 48	6.18	K5III
HR 723			BD+22 354	15385	75398						02 29 13.6	+23 28 08	6.19	A5m
HR 728			BD+24 358	15524	75407	2171			1904		02 30 32.4	+25 14 06	5.92	F6IV	4.5	113.1	D:ADS 1904AB binary; B, 11v.
HR 729		26	BD+19 365	15550	92979	2172		D		UU Ari	02 30 38.4	+19 51 19	6.15	A9V			D:Suspected occultation double.,S:Also classified A9III.,VAR:Delta Sct 6.11 - 6.15V, 0.080d.
HR 731		27	BD+17 380	15596	92983	1069					02 30 54.4	+17 42 14	6.23	G5III-IV
HR 741		29	BD+14 419	15814	92998	2176					02 32 54.1	+15 02 05	6.04	F8V
HR 763		31	BD+11 360	16234	93022	2179		D			02 36 37.9	+12 26 51	5.68	F7V	0.1	0.0	D:Sep. 0.021".
HR 764		30	BD+24 375	16232	75470				1982 B		02 36 57.7	+24 38 54	7.09	F4V	0.6	38.3	D:CPM with HR 765. HR 764 formerly misidentified as the SB = HR 765. Data for HR 764 and 765 have frequently been,D:interchanged.
HR 765		30	BD+24 376	16246	75471				1982 A		02 37 00.5	+24 38 51	6.50	F6III	0.6	38.3	D:CPM with HR 764.,G:Hyades group.,SB:ADS 1982A, 1.1095d, K 22.4k/s, V0 +14.4k/s, asini 0.341.
HR 773	ν	32	BD+21 362	16432	75495	89					02 38 49.0	+21 57 41	5.43	A7V
HR 782		33	BD+26 443	16628	75510				2033		02 40 41.1	+27 03 39	5.30	A3V	4.2	28.6	D:CPM.
HR 793	μ	34	BD+19 403	16811	93062				2062		02 42 22.0	+20 00 42	5.69 R	A0Vnp:	0.8	0.1	D:AB 6.2, 12.2v, 19" about 6y. Occultations indicate A is triple system, 7.0v A1, at 0.06", and 8.0v at 0.2". Aa,D:resolved by speckle interferometry, sep. 0.045" 1981.68, 0.040" 1981.69.,S:Lambda Boo star, Mg 4481 wk:
HR 797			BD+10 360	16861	93067					899	02 42 28.9	+10 44 30	6.30	A2V			G:UMa stream.,VAR:Delta Sct?
HR 801		35	BD+27 424	16908	75532	94					02 43 27.1	+27 42 26	4.66	B3V			G:Cas-Tau OB1.,SB:490d. Short period 2.6d not confirmed. K 8.8, V0 +13.0, asini 58.7.
HR 803			BD+25 441	16955	75539				2082		02 43 51.2	+25 38 17	6.35	A2Vp:	4.1	2.9	D:AB CPM.,S:Lambda Boo star, Mg 4481 wk:
HR 808		36	BD+17 426	17017	93081	2190					02 44 19.1	+17 45 50	6.46	K2III			G:Wolf 630 group.
HR 809	ο	37	BD+14 457	17036	93082						02 44 32.9	+15 18 42	5.77	B9Vn
HR 812		38	BD+11 377	17093	93083					UV Ari	02 44 57.6	+12 26 45	5.18	A7III-IV			VAR:Delta Sct 5.18 - 5.22V, 0.0355d with overtones of 0.046 and 0.061d.
HR 824		39	BD+28 462	17361	75578		I				02 47 54.5	+29 14 50	4.51	K1.5III
HR 828		40	BD+17 442	17459	93118		I	D		937	02 48 32.1	+18 17 01	5.82	K1III	0.0	0.2	D:Suspected occultation double, 6.8, 6.8v, sep. 0.2".,G:Probable Hyades group.
HR 830			BD+24 396	17471	75588					VZ Ari	02 48 45.9	+25 11 17	5.86 R	A0V			S:Also classified ApSi.,VAR:Alpha CV, 5.82 - 5.89V.
HR 836	π	42	BD+16 355	17543	93127				2151	944	02 49 17.5	+17 27 51	5.22	B6V	3.0	0.0	D:AB CPM. B 8.8v, A0Vp at 3.2", RV -21k/s, probably optical; C 10.72V, +0.60(B-V), +0.60(U-B), F8V at 25". A is close SB,D:pair with computed sep. 0.00004".,SB:ADS 2151A, 3.854d, K 24.8k/s, V0 +7.8k/s, asini 1.31.
HR 838		41	BD+26 471	17573	75596	100			2159	951	02 49 59.0	+27 15 38	3.63	B8Vn	4.8	124.9	D:Optical system.,G:Pleiades group.
HR 847	σ	43	BD+14 480	17769	93144	1079					02 51 29.6	+15 04 55	5.49	B7V
HR 856			BD+15 400	17918	93164						02 53 11.7	+16 29 00	6.31	F5III
HR 867	ρ²	45	BD+17 457	18191	93189					RZ Ari	02 55 48.5	+18 19 54	5.91	M6-III:			N:Rho1 Fl 44, Rho2 Fl 45, Rho3 Fl 46 Ari are, respectively, HD 18091 (6.93v, A3), HR 867 and 869. HR 869 is,N:also called simply Rho Ari.,R:Occultation diam. = 0.0095 - 0.012".,VAR:SRb 5.62 - 6.01V, 30d.
HR 869	ρ³	46	BD+17 458	18256	93195	2204					02 56 26.1	+18 01 23	5.63	F6V			SB:3507d, K 6.7k/s, V0 +12.1k/s, asini 308. Orbit questioned by Morbey and Griffin (1987, ApJ, 317, 343).,SB:Unresolved by speckle interferometry 1978.96.
HR 878		47	BD+20 480	18404	75662	1081					02 58 05.2	+20 40 07	5.80	F5IV			G:Hyades group.
HR 887	ε	48	BD+20 484	18519	75673				2257 B	1001	02 59 12.7	+21 20 25	4.63	A2V s	0.3	1.5	D:Binary with HR 888. Mag. and colors for combined light.,DYN:0.012".,VAR:Uncertain if HR 887 or 888 is the variable suspect.
HR 888	ε	48	BD+20 484	18520	75673				2257 A	1001	02 59 12.7	+21 20 25	4.63	A2V s	0.3	1.5	D:A, 5.25H; B = HR 887, 5.55H; C, 12.7v at 146".,DYN:0.012".
HR 902			BD+10 401	18700	93232	2213	I				03 00 44.1	+10 52 13	5.95	K6
HR 905		49	BD+25 477	18769	75693	2214				1021	03 01 54.1	+26 27 44	5.90	A3m
HR 916			BD+27 468	18928	75709						03 03 30.3	+28 16 11	6.36	F0V
HR 924			BD+15 430	19080	93260						03 04 40.7	+15 51 22	6.49 R	K3III
HR 927		52	BD+24 431	19134	75723				2336 A		03 05 26.7	+25 15 19	6.80	B7V	0.0	0.2	D:Binary with HR 928. Colors for combined light. AB, 227y, a = 0.470". Triple system with C, 10.8v at 5".,RV:Probably blended with HR 928.
HR 928		52	BD+24 431	19135	75723				2336 B		03 05 26.7	+25 15 19	7.00	B7V	0.0	0.2	D:See HR 927.,RV:Probably blended with HR 927.
HR 931			BD+12 436	19270	93276	2220					03 06 23.7	+13 11 14	5.62	K3III
HR 938		53	BD+17 493	19374	93284			D		UW Ari	03 07 25.7	+17 52 48	6.11	B1.5V	0.0	0.0	D:Sep. 0.03".,M:Runaway star from Ori OB1 association at 59k/s. Presumably originated in Ori 1 assoc. Its space vel. is twice that of,M:HR 1712 = AE Aur and opposite that of HR 2688. These three stars and HR 1996 (Mu Col) appear to be receding from an,M:HII shell of about 110000 solar masses expanding at 10k/s.,SB:0.15275d. Amp. and V0 variable.,VAR:Beta C 6.10 - 6.23V, 0.15275d. Possibly a SN 4.9 million yrs. ago.
HR 940		54	BD+18 414	19460	93293		I				03 08 21.2	+18 47 42	6.27	M0III			R:Diam. 0.0021".
HR 944		55	BD+28 499	19548	75757	1088					03 09 36.7	+29 04 37	5.72	B8III			G:Member of the local association (Pleiades group).
HR 945			BD+27 480	19600	75762						03 10 08.8	+27 49 12	6.42	A0V v			VAR:Constant light but large H-line variation.
HR 946			BD+26 516	19637	75771						03 10 27.0	+26 53 47	6.02	K3III
HR 948			BD+11 445	19698	93320			D			03 10 38.9	+11 52 21	5.98	B8V			D:Suspected occultation double.
HR 951	δ	57	BD+19 477	19787	93328	114	I			1066	03 11 37.8	+19 43 36	4.35	K2III v			G:Hyades group.,N:Botein.
HR 952			BD+12 452	19789	93327			D			03 11 21.9	+13 02 52	6.12	K0IIIp			D:Suspected occultation double.
HR 954		56	BD+26 523	19832	75788					SX Ari	03 12 14.2	+27 15 25	5.79	B9pSi v			RV:Period 0.728d probably rotation period. Earlier determination vsini 94k/s.,VAR:SX Ari 5.67 - 5.81V, 0.7278925d. Spectral variations (SiII, HeI, same period). Possible 30 min Sp. var.,VAR:suggesting star spots related to magnetic field. Silicon abundance varies 10 to 100 times solar, and magnesium 0.03 to,VAR:10 times solar.
HR 971			BD+30 512	20149	56285						03 15 20.5	+30 33 24	5.52 R	A1V s
HR 972	ζ	58	BD+20 527	20150	75810	1089					03 14 54.1	+21 02 40	4.89	A1V
HR 995		59	BD+26 540	20618	75863						03 19 55.8	+27 04 16	5.90	G6IV
HR 999			BD+28 516	20644	75871	2234	I				03 20 20.4	+29 02 54	4.47	K2II-III
HR 1000		60	BD+25 536	20663	75875						03 20 25.6	+25 39 46	6.12	gK3
HR 1005	τ¹	61	BD+20 543	20756	75886	1094		W			03 21 13.6	+21 08 49	5.28	B5IV	2.5	0.2	D:Suspected of being double or triple by Tebbutt in 1893. Components 5.4, 7.9v, sep. 0.15", and 8.4v at 0.67".,G:Cas-Tau OB1.
HR 1012		62	BD+27 500	20825	75892						03 22 11.9	+27 36 27	5.52	G5III
HR 1015	τ²	63	BD+20 551	20893	75899		I				03 22 45.2	+20 44 31	5.09	K3III
HR 1022		64	BD+24 481	21017	75912	2240	I				03 24 18.5	+24 43 27	5.50	gK4
HR 1027		65	BD+20 556	21050	75915						03 24 26.1	+20 48 13	6.08	A1V
HR 1048		66	BD+22 495	21467	75945				2552		03 28 26.6	+22 48 15	6.03	K0IV	1.4	0.0	D:ADS 2552A is close binary, 6.3, 7.7v, sep. 0.010". AB binary; C, 13v at 148".

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

Aries / Yale Bright Star Catalog (HR)

Legend

References