Star in the constellation Columba
For other stars with this Bayer designation , see ν Columbae .
Nu Columbae is a solitary star in the southern constellation of Columba . It can be seen with the naked eye, having an apparent visual magnitude of 5.31. With an annual parallax shift of 24.51 mas , it is estimated to lie about 133 light years from the Sun .
This star has a stellar classification of F5 V, indicating that it is an F-type main sequence star that is generating energy through the thermonuclear fusion of hydrogen into helium in its core region. It has about 1.65 times the mass of the Sun and 1.6 times the Sun's radius . X-ray emission has been detected from this star, with an estimated luminosity of 1.6×10 erg/s . It is about 1.8 billion years old and is spinning with a projected rotational velocity of 27.2 km/s. The star is radiating about 10 times the solar luminosity from its outer atmosphere at an effective temperature of 6,473 K.
References
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^ Pasinetti Fracassini, L. E.; et al. (February 2001), "Catalogue of Apparent Diameters and Absolute Radii of Stars (CADARS) - Third edition - Comments and statistics", Astronomy and Astrophysics , 367 (2): 521–524, arXiv :astro-ph/0012289 , Bibcode :2001A&A...367..521P , doi :10.1051/0004-6361:20000451 , S2CID 425754 .
^ McDonald, I.; et al. (2012), "Fundamental Parameters and Infrared Excesses of Hipparcos Stars", Monthly Notices of the Royal Astronomical Society , 427 (1): 343–57, arXiv :1208.2037 , Bibcode :2012MNRAS.427..343M , doi :10.1111/j.1365-2966.2012.21873.x , S2CID 118665352 .
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Balachandran, Suchitra (May 1, 1990), "Lithium depletion and rotation in main-sequence stars", Astrophysical Journal, Part 1 , 354 : 310–332, Bibcode :1990ApJ...354..310B , doi :10.1086/168691 .
"nu.02 Col -- Star" , SIMBAD Astronomical Database , Centre de Données astronomiques de Strasbourg , retrieved 2016-12-30.
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 .
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