Star in the constellation Cepheus
Kappa Cephei , Latinized from κ Cephei, is a binary star [ 10] system in the northern circumpolar constellation of Cepheus . It is visible to the naked eye as a faint, blue white-hued point of light with an apparent visual magnitude is 4.39.[ 11] The system is located approximately 323–326 light years distant from the Sun, based on parallax .
The two gravitationally-bound members of this system had an angular separation of 7.3″ along a position angle of 120°, as of 2015.[ 11] The primary, designated component A, has a stellar classification of B9III,[ 3] matching a blue giant . The magnitude 8.34 secondary, component B, is an A-type main-sequence star of class A7V.[ 3] A third star of 10th magnitude, BD+77 763, is listed as component C in the Washington Double Star Catalog although it is a background object unrelated to the other two.
[ 11]
References
^ a b c d e Brown, A. G. A. ; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties" . Astronomy & Astrophysics . 616 . A1. arXiv :1804.09365 . Bibcode :2018A&A...616A...1G . doi :10.1051/0004-6361/201833051 . Gaia DR2 record for this source at VizieR .
^ a b c Hoffleit, D.; Warren, W. H. (1995). "VizieR On-line Data Catalog: Bright Star Catalogue". VizieR On-line Data Catalog: V/50. Originally Published in: 1964BS....C......0H . 5050 (5th Revised ed.). Bibcode :1995yCat.5050....0H .
^ a b c Murphy, R. E. (1969). "A spectroscopic investigation of visual binaries with B-type primaries" . The Astronomical Journal . 74 : 1082. Bibcode :1969AJ.....74.1082M . doi :10.1086/110908 .
^ a b c Anderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation", Astronomy Letters , 38 (5): 331, arXiv :1108.4971 , Bibcode :2012AstL...38..331A , doi :10.1134/S1063773712050015 , S2CID 119257644 .
^ a b Evans, D. S. (1967). "The Revision of the General Catalogue of Radial Velocities". Determination of Radial Velocities and Their Applications . 30 : 57. Bibcode :1967IAUS...30...57E .
^ a b c d e f Brown, A. G. A. ; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties" . Astronomy & Astrophysics . 616 . A1. arXiv :1804.09365 . Bibcode :2018A&A...616A...1G . doi :10.1051/0004-6361/201833051 . Gaia DR2 record for this source at VizieR .
^ a b David, Trevor J.; Hillenbrand, Lynne A. (2015). "The Ages of Early-type Stars: Strömgren Photometric Methods Calibrated, Validated, Tested, and Applied to Hosts and Prospective Hosts of Directly Imaged Exoplanets". The Astrophysical Journal . 804 (2): 146. arXiv :1501.03154 . Bibcode :2015ApJ...804..146D . doi :10.1088/0004-637x/804/2/146 . S2CID 33401607 .
^ a b c Fitzpatrick, E. L.; Massa, D. (March 2005). "Determining the Physical Properties of the B Stars. II. Calibration of Synthetic Photometry". The Astronomical Journal . 129 (3): 1642– 1662. arXiv :astro-ph/0412542 . Bibcode :2005AJ....129.1642F . doi :10.1086/427855 . S2CID 119512018 .
^ "kap Cep" . SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 2019-09-11 .
^ Eggleton, P. P.; Tokovinin, A. A. (2008). "A catalogue of multiplicity among bright stellar systems" . Monthly Notices of the Royal Astronomical Society . 389 (2): 869. arXiv :0806.2878 . Bibcode :2008MNRAS.389..869E . doi :10.1111/j.1365-2966.2008.13596.x . S2CID 14878976 .
^ a b c Mason, Brian D.; et al. (2001). "The 2001 US Naval Observatory Double Star CD-ROM. I. The Washington Double Star Catalog" . The Astronomical Journal . 122 (6): 3466. Bibcode :2001AJ....122.3466M . doi :10.1086/323920 .