Star in the constellation Auriga
Omicron Aurigae , Latinized from ο Aurigae , is the Bayer designation for an astrometric binary star system in the northern constellation of Auriga . With an apparent visual magnitude of 5.47, it is faintly visible to the naked eye. Based upon an annual parallax shift of 7.89 ± 0.84 mas , it is approximately 413 light-years (127 parsecs ) distant from Earth. The star is a member of the Ursa Major stream of co-moving stars.
The visible component is a chemically peculiar star with a stellar classification of A1 Cr Eu; meaning this is an A-type star with a spectrum that shows abnormally high abundances of chromium (Cr) and europium (Eu). A magnetic field has been detected and it is a source of X-ray emission with a luminosity of: log Lx = 29.1. It is spinning with a projected rotational velocity of 29 km/s and is radiating 95 times the Sun's luminosity from its photosphere at an effective temperature of 8,660 K.
References
^ van Leeuwen, F. (2007), "Validation of the new Hipparcos reduction", Astronomy and Astrophysics , 474 (2): 653–664, arXiv :0708.1752 , Bibcode :2007A&A...474..653V , doi :10.1051/0004-6361:20078357 , S2CID 18759600 .
^ Johnson, H. L.; et al. (1966), "UBVRIJKL photometry of the bright stars", Communications of the Lunar and Planetary Laboratory , 4 (99): 99, Bibcode :1966CoLPL...4...99J .
^ Renson, P.; Manfroid, J. (May 2009), "Catalogue of Ap, HgMn and Am stars" , Astronomy and Astrophysics , 498 (3): 961–966, Bibcode :2009A&A...498..961R , doi :10.1051/0004-6361/200810788 .
Deutschman, W. A.; et al. (February 1976), "The galactic distribution of interstellar absorption as determined from the Celescope catalog of ultraviolet stellar observations and a new catalogue of UBV, Hbeta photoelectric observations", Astrophysical Journal Supplement Series , 30 : 97–225, Bibcode :1976ApJS...30...97D , doi :10.1086/190359 .
de Bruijne, J. H. J.; Eilers, A.-C. (October 2012), "Radial velocities for the HIPPARCOS-Gaia Hundred-Thousand-Proper-Motion project", Astronomy & Astrophysics , 546 : 14, arXiv :1208.3048 , Bibcode :2012A&A...546A..61D , doi :10.1051/0004-6361/201219219 , S2CID 59451347 , A61.
^ 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 .
^ Moiseeva, A. V.; et al. (January 2019), "Fundamental Parameters of CP Stars Observed at the 6-m Telescope. I. Observations in 2009–2011", Astrophysical Bulletin , 74 (1): 62–65, Bibcode :2019AstBu..74...62M , doi :10.1134/S1990341319010061 .
^ McDonald, I.; et al. (2012), "Fundamental parameters and infrared excesses of Hipparcos stars", Monthly Notices of the Royal Astronomical Society , 427 (1): 343–357, arXiv :1208.2037 , Bibcode :2012MNRAS.427..343M , doi :10.1111/j.1365-2966.2012.21873.x , S2CID 118665352 .
"omi Aur" . SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 2017-06-28.
Makarov, V. V.; Kaplan, G. H. (May 2005), "Statistical Constraints for Astrometric Binaries with Nonlinear Motion" (PDF), The Astronomical Journal , 129 (5): 2420–2427, Bibcode :2005AJ....129.2420M , doi :10.1086/429590 , archived from the original on September 24, 2017.
^ Panzera, M. R.; et al. (August 1999), "X-ray emission from A0-F6 spectral type stars", Astronomy and Astrophysics , 348 : 161–169, arXiv :astro-ph/9906221 , Bibcode :1999A&A...348..161P .
Royer, F.; et al. (October 2002), "Rotational velocities of A-type stars in the northern hemisphere. II. Measurement of v sin i", Astronomy and Astrophysics , 393 : 897–911, arXiv :astro-ph/0205255 , Bibcode :2002A&A...393..897R , doi :10.1051/0004-6361:20020943 , S2CID 14070763 .
External links
Categories :
Omicron Aurigae
Add topic
Text is available under the Creative Commons Attribution-ShareAlike License. Additional terms may apply.
**DISCLAIMER** We are not affiliated with Wikipedia, and Cloudflare.
The information presented on this site is for general informational purposes only and does not constitute medical advice.
You should always have a personal consultation with a healthcare professional before making changes to your diet, medication, or exercise routine.
AI helps with the correspondence in our chat.
We participate in an affiliate program. If you buy something through a link, we may earn a commission 💕
↑