Binary star system in the constellation Fornax
Omega Fornacis , which is Latinized from ω Fornacis, is a wide binary star system in the southern constellation of Fornax . It has a blue-white hue and is faintly visible to the naked eye as a fifth-magnitude star. The system lies at a distance of approximately 470 light years from the Sun based on parallax , and is drifting further away with a radial velocity of +10 km/s.
The dual nature of this system was discovered in 1836 by John Herschel . As of 2013, the two components had an angular separation of 11.0″ along a position angle of 246°. This corresponds to a projected separation of 1,520 AU .
The magnitude 4.95 primary, designated component A, is a chemically peculiar B-type main-sequence star with a stellar classification of B9V It has 3.4 times the Sun's mass and is radiating around 268 times the luminosity of the Sun from its photosphere at an effective temperature of 10,910 K. Component B, the magnitude 7.71 secondary, is an A-type main-sequence star with a class of A3V. It is smaller than the primary, but has a higher projected rotational velocity .
References
^ 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 .
^ Mason, B. D.; et al. (2014), "The Washington Visual Double Star Catalog" , The Astronomical Journal , 122 (6): 3466, Bibcode :2001AJ....122.3466M , doi :10.1086/323920 , retrieved 2015-07-22
^ Zorec, J.; Royer, F. (January 2012), "Rotational velocities of A-type stars. IV. Evolution of rotational velocities", Astronomy & Astrophysics , 537 : A120, arXiv :1201.2052 , Bibcode :2012A&A...537A.120Z , doi :10.1051/0004-6361/201117691 , S2CID 55586789 .
^ Houk, Nancy (1979). Michigan catalogue of two-dimensional spectral types for the HD stars . Vol. 3. Ann Arbor, Michigan: Dept. of Astronomy, University of Michigan. Bibcode :1982mcts.book.....H .
^ Hoffleit, D.; Warren, Jr., W. H. (1991). "VizieR Detailed Page" . Bright Star Catalogue (5th Revised ed.). CDS . Retrieved 2012-07-13.
^ 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 .
^ Howe, K. S.; Clarke, C. J. (January 2009). "An analysis of v sin (i) correlations in early-type binaries" . Monthly Notices of the Royal Astronomical Society . 392 (1): 448–454. Bibcode :2009MNRAS.392..448H . doi :10.1111/j.1365-2966.2008.14073.x .
^ Corbally, C. J. (1984). "Close visual binaries. I - MK classifications". Astrophysical Journal Supplement Series . 55 : 657. Bibcode :1984ApJS...55..657C . doi :10.1086/190973 .
^ Zorec, J.; et al. (2009). "Fundamental parameters of B supergiants from the BCD system. I. Calibration of the (λ_1, D) parameters into Teff". Astronomy and Astrophysics . 501 (1): 297–320. arXiv :0903.5134 . Bibcode :2009A&A...501..297Z . doi :10.1051/0004-6361/200811147 . S2CID 14969137 .
"ome For" . SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 2019-10-29.
Eggleton, P. P.; Tokovinin, A. A. (September 2008). "A catalogue of multiplicity among bright stellar systems" . Monthly Notices of the Royal Astronomical Society . 389 (2): 869–879. arXiv :0806.2878 . Bibcode :2008MNRAS.389..869E . doi :10.1111/j.1365-2966.2008.13596.x . S2CID 14878976 . Vizier catalog entry
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