Catalogues

Catalogue

Constellation

Canes Venatici / 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 4666		2	BD+41 2284	106690	44097	458	I		8489		12 16 07.6	+40 39 37	5.66	M1III+F7V	3.1	11.4	D:Binary. Companion 8.77V, +0.57(B-V), +0.09(U-B), F7V.
HR 4690		3	BD+49 2130	107274	44127	1316	I				12 19 48.7	+48 59 03	5.29	M0III
HR 4715		4	BD+43 2218	107904	44155	2993				AI CVn	12 23 47.0	+42 32 34	6.06	F3III-IV			G:In Hyades group.,SB:0.1707d.,VAR:Delta Sct 5.89 - 6.15V. Multiple periods 0.2085, 0.1529, 0.1259 and 0.1158d.
HR 4716		5	BD+52 1626	107950	28366	2994	I			Var	12 24 01.5	+51 33 44	4.80	G6IIIBa0.2			VAR:E? Amp. 0.067V.
HR 4728		6	BD+39 2521	108225	63000	461	I				12 25 50.9	+39 01 07	5.02	G9III
HR 4761		7	BD+52 1631	108845	28407			W			12 30 02.9	+51 32 08	6.21	F6-8V	2.8	229.0
HR 4783			BD+34 2332	109317	63070	1322	I				12 33 38.9	+33 14 51	5.42	K0IIICN-1
HR 4784			BD+34 2333	109345	63072						12 33 47.4	+33 23 05	6.24	K0III
HR 4785	β	8	BD+42 2321	109358	44230	470	I	S		5725	12 33 44.5	+41 21 27	4.26	G0V			M:Probable nearby star.,N:Chara is the name assigned either to this star or, more generally, to the "southern hound" of the constellation Canes,N:Venatici; the northern "hound" is called Asterion, a name not generally assigned any particular star.,SB:2429.9d, K 2.6k/s, V0 +6.5k/s, asini 75.7. Orbit questioned by Morbey and Griffin (1987, ApJ, 317, 343).,SB:Resolved by speckle interferometry 1978.40, sep. 0.110"; however, unresolved on numerous other occasions, so measure,SB:must be confirmed.,VAR:Beta CVn amp. 0.05V.
HR 4811		9	BD+41 2312	109980	44265						12 38 46.3	+40 52 28	6.37	A7Vn
HR 4816			BD+36 2295	110066	63118	3013				AX CVn	12 39 16.9	+35 57 07	6.45	A0pSrCrEu			S:Unusually strong CrI and FeI lines. Magnetic star. 73 Dra type.,VAR:Alpha CV 6.32 - 6.55V, 4900:d.
HR 4843			BD+44 2221	110834	44307						12 44 27.1	+44 06 11	6.33	F6IV
HR 4845		10	BD+40 2570	110897	63177						12 44 59.5	+39 16 44	5.95	G0V
HR 4846			BD+46 1817	110914	44317	1327	I			Y CVn	12 45 07.8	+45 26 25	4.99	C7I			S:Infrared spectra show CO, CN and C2 molecules.,VAR:SRb 7.4 - 10.0p, 158.0d, some cycles 250 and 90d. Possible secondary 2000 - 2200d.
HR 4866		11	BD+49 2163	111421	44332						12 48 41.8	+48 28 01	6.27	A6m
HR 4875			BD+38 2373	111604	63217					5983	12 50 10.7	+37 31 01	5.89	A3V			VAR:Delta Sct? 5.9 - 5.94v.
HR 4904			BD+34 2369	112171	63244	3027					12 54 13.1	+33 32 04	6.26	A7IV
HR 4909			BD+47 2003	112264	44383	3030	I			TU CVn	12 54 56.5	+47 11 48	5.84	M5III			VAR:SRb 5.55 - 6.6V, 7.2 - 7.7p, 50d.
HR 4914	α¹	12	BD+39 2580	112412	63256				8706 B		12 56 00.4	+38 18 53	5.60	F0V	2.7	19.4	D:Binary with HR 4915.,DYN:0.015".,G:Hyades group.
HR 4915	α²	12	BD+39 2580	112413	63257	485	I		8706 A	Alp2 CVn	12 56 01.7	+38 19 06	2.90	A0pSiEuHg	2.7	19.4	D:Binary with HR 4914.,DYN:0.015".,G:Hyades group.,N:COR CAROLI.,R:Radius relative to Sun = 4.1.,S:Oxygen deficient relative to magnesium. A slight underabundance of Mg. Strong Si and Eu lines. Also classified,S:A0IIIp, A1IV-Vp (Si v. st., Ca v. wk.).,VAR:ADS 8706A, Alpha CV 2.84 - 2.98V, 2.78 - 2.81B, 5.46939d. The prototype star. Var. magnetic field with same rotation,VAR:period.
HR 4919			BD+46 1833	112570	44398						12 57 07.7	+46 10 37	6.12	K0III-IV
HR 4943		14	BD+36 2337	113797	63338	1337				6089	13 05 44.5	+35 47 56	5.25	B9V			RV:Previous estimates vsini from 0 to 170:k/s.,VAR:5.1 - 5.3v. Period of some hours?
HR 4945			BD+46 1847	113847	44465	1338	I		8775		13 05 52.3	+45 16 07	5.63	K1III	5.4	2.9
HR 4964			BD+38 2407	114357	63372						13 09 38.7	+37 25 23	6.02	K3III
HR 4967		15	BD+39 2611	114376	63374				8805 BC		13 09 42.0	+38 32 02	6.28	B7III	0.3	284.4	D:ADS 8805BC. Binary? C, 11.2 at 1". A is HR 4971, not CPM. ADS and IDS differ on naming of the components. IDS,,D:adopted here, is the more consistent with FGW Struve's early discovery.
HR 4971		17	BD+39 2614	114447	63380	491			8805 A		13 10 03.2	+38 29 56	5.91	A9III-IV	0.3	284.4	S:Also classified F0V.
HR 4997			BD+40 2633	115004	44519		I				13 13 43.0	+40 09 10	4.92	G8IIIaCN0.5
HR 5004		19	BD+41 2374	115271	44531						13 15 32.0	+40 51 19	5.79	A7V
HR 5017		20	BD+41 2380	115604	44549	494				AO CVn	13 17 32.5	+40 34 21	4.73	F3III			G:Hyades group?,S:MgII 4481 anomalously strong.,SB:Amp. 1.5k/s, 0.135d or 0.176d.,VAR:Delta Sct 4.70 - 4.75V, 0.12168d. Var. amp.?
HR 5022			BD+34 2410	115723	63462		I				13 18 27.8	+34 05 53	5.82	K4.5III
HR 5023		21	BD+50 1994	115735	44556	3063				BK CVn	13 18 14.5	+49 40 55	5.15	A0V			S:Also classified ApSi.,VAR:Alpha CV, amp. 0.04V, 0.767d.
HR 5025			BD+35 2435	115810	63468	3064			8861 D		13 19 04.2	+35 07 41	6.02	F0IV	3.6	319.0
HR 5032		23	BD+40 2647	116010	44570	1346	I				13 20 19.0	+40 09 02	5.60	K1III
HR 5045			BD+44 2269	116303	44582					6210	13 22 03.8	+43 54 11	6.35	A7m
HR 5052			BD+37 2404	116581	63514		I			6220	13 23 54.0	+37 02 02	6.07	M3III
HR 5067			BD+46 1868	116957	44611						13 26 16.6	+46 01 41	5.88	gK0
HR 5077			BD+41 2400	117261	44621						13 28 26.2	+40 43 47	6.47	G8III
HR 5079			BD+51 1846	117281	28766						13 28 11.7	+50 35 14	6.80 R	F1IV
HR 5083			BD+51 1847	117361	28771						13 28 45.7	+50 43 06	6.43	F0IV			C:IR source?,S:Also classified F5V, Sr enhanced.
HR 5096			BD+42 2405	117710	44637						13 31 15.8	+42 06 22	6.08	K2III
HR 5108			BD+39 2658	118156	63616				8956		13 34 21.8	+38 47 21	6.37	F0IV	4.3	30.6	D:Optical.
HR 5110			BD+37 2426	118216	63623	502				BH CVn	13 34 47.8	+37 10 57	4.98	F2IV			SB:2.6132d, K 9.5k/s, V0 +6.4k/s, asini 0.341. Eker and Doherty (1987, MNRAS, 228, 869) observed double lines at high,SB:resolution and provide and alternate orbit. A primary temperature of 6750 K is estimated from Fe/C line ratio, while,SB:equivalent widths of CaI and FeI lines from K-type secondary give 4500-5000 K. Implied spectral type of secondary is,SB:K2IV.,VAR:RS 4.94 - 5.01V, 2.6131738d. Probable reflection effect.
HR 5112		24	BD+49 2227	118232	44668	3083				6322	13 34 27.3	+49 00 58	4.70	A5V			S:Shell star, but shell seems to have disappeared in 1981, 1983.,VAR:Delta Sct?
HR 5116			BD+44 2285	118295	44675	1353					13 35 14.1	+44 11 49	6.84	A7-F0III
HR 5127		25	BD+37 2433	118623	63648				8974		13 37 27.6	+36 17 42	4.82	A7III	2.0	1.7	D:AB 5.01 A7III, 6.91 F0V, 240.0y, a = 1.091" or 220.4y, a = 1.205". Combined mag., colors.,DYN:0.017".
HR 5143			BD+31 2526	119035	63676						13 40 15.6	+31 00 43	6.21	G5II:
HR 5145			BD+28 2248	119081	82944			W			13 40 39.1	+28 03 55	6.23	K3III	3.3	91.2
HR 5160			BD+42 2431	119445	44720						13 42 28.8	+41 40 27	6.30	G6III
HR 5161			BD+35 2474	119458	63701	3089					13 42 43.4	+34 59 20	5.98	G5III			SB:149.72d, K 20.8k/s, V0 -7.7k/s, asini 42.2.
HR 5179			BD+41 2424	120047	44742						13 46 13.5	+41 05 19	5.87	A5V
HR 5180			BD+39 2678	120048	63735						13 46 19.0	+38 30 14	5.94	G9III
HR 5186			BD+39 2680	120164	63739	3094		W			13 46 59.8	+38 32 34	5.50	K0III+F8V	3.2	71.3
HR 5195			BD+31 2547	120420	63760	3096					13 48 38.7	+31 11 25	5.62	K0III
HR 5199			BD+40 2694	120499	63763		I			R CVn	13 48 57.2	+39 32 34	7.40	M6IIIe v			S:Also classified M5.5e-M9e.,VAR:M 6.5 - 12.9v, 328.53d. Period varies.
HR 5204			BD+37 2457	120600	63772						13 49 45.0	+36 37 58	6.38 R	A7IV-V
HR 5214			BD+35 2492	120818	63779						13 51 04.5	+34 46 21	6.65	A5IV			G:Sirius group; UMa stream.
HR 5215			BD+35 2493	120819	63781		I			6468	13 51 09.2	+34 39 52	5.87	M2III
HR 5219			BD+35 2496	120933	63793	3102	I			AW CVn	13 51 47.5	+34 26 39	4.74	K5III			VAR:SR? 4.72 - 4.81V.
HR 5229			BD+29 2464	121164	83055	3106					13 53 10.3	+28 38 53	5.90	A7V
HR 5245			BD+32 2411	121682	63837	1360					13 56 10.5	+32 01 57	6.32	F4IV-V
HR 5271			BD+46 1922	122675	44858	3115					14 02 12.2	+45 45 13	6.27	K2III

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

Canes Venatici / Yale Bright Star Catalog (HR)

Legend

References