Catalogues

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)

References