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Star in the constellation Vela
This article is about C Velorum. For c Velorum, see
HD 78004 .
HR 3407 is a single[ 10] star in the southern constellation of Vela . It has the Bayer designation C Velorum ; HR 3407 is the designation in the Bright Star Catalogue [ 9] apparent visual magnitude of 5.01.[ 2] light years based on parallax measurements, and it is drifting further away with a radial velocity of 4 km/s.[ 1]
This object is an aging K-type supergiant star with a stellar classification of K1.5Ib.[ 3] [ 6] mass of the Sun and has expanded to around 71[ 1] Sun's radius . The latter is equivalent to 0.33 AU , or about one third the distance from the Sun to the Earth. It is spinning with a projected rotational velocity of 4.1.[ 8] [ 4] luminosity of the Sun from its enlarged photosphere at an effective temperature of 4,324 K.[ 1]
^ a b c d e f g h i 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 d Hoffleit, D.; Warren, W. H. (1995), "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 Keenan, Philip C.; McNeil, Raymond C. (1989), "The Perkins Catalog of Revised MK Types for the Cooler Stars", The Astrophysical Journal Supplement Series , 71 : 245, Bibcode :1989ApJS...71..245K , doi :10.1086/191373 , S2CID 123149047 . ^ a b Koen, Chris; Eyer, Laurent (2002), "New periodic variables from the Hipparcos epoch photometry", Monthly Notices of the Royal Astronomical Society , 331 (1): 45–59, arXiv :astro-ph/0112194 Bibcode :2002MNRAS.331...45K , doi :10.1046/j.1365-8711.2002.05150.x S2CID 10505995 . ^ 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 Stello, D.; et al. (2008), "Oscillating K Giants with the WIRE Satellite: Determination of Their Asteroseismic Masses", The Astrophysical Journal Letters , 674 (1): L53–L56, arXiv :0801.2155 Bibcode :2008ApJ...674L..53S , doi :10.1086/528936 , S2CID 15094067 . ^ a b c Messineo, M.; Brown, A. G. A. (2019). "A Catalog of Known Galactic K-M Stars of Class I Candidate Red Supergiants in Gaia DR2" . The Astronomical Journal . 158 (1): 20. arXiv :1905.03744 Bibcode :2019AJ....158...20M . doi :10.3847/1538-3881/ab1cbd S2CID 148571616 . ^ a b c d Lèbre, A.; de Laverny, P.; Do Nascimento, J. D. Jr.; de Medeiros, J. R. (May 2006), "Lithium abundances and rotational behavior for bright giant stars" (PDF) , Astronomy and Astrophysics , 450 (3): 1173–1179, Bibcode :2006A&A...450.1173L , doi :10.1051/0004-6361:20053485 ^ a b "C Vel" . SIMBAD Centre de données astronomiques de Strasbourg . Retrieved 2019-12-04 .^ 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 .
