Phi Aurigae
Star in the constellation Auriga
φ Aurigae in optical light
Phi Aurigae , Latinized from φ Aurigae, is a giant star in the northern constellation of Auriga . It is faintly visible to the naked eye with an apparent visual magnitude of 5.089.[ 2] It lies 10′ from another faint naked-eye star HD 35520 , between the three open clusters M36 and M38 , and NGC 1893 .
The distance to this star, as determined from parallax measurements, is approximately 480 light-years (150 parsecs ) with a 10 light-year margin of error .[ 9] This is an evolved giant star with a stellar classification of K3 IIIp[ 3] and an estimated radius equal to 34 times the radius of the Sun. The outer envelope has an effective temperature of 4,222 K,[ 6] giving it the cool orange-hued glow of a K-type star .
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 d Jennens, P. A.; Helfer, H. L. (September 1975), "A new photometric metal abundance and luminosity calibration for field G and K giants.", Monthly Notices of the Royal Astronomical Society , 172 (3): 667– 679, Bibcode :1975MNRAS.172..667J , doi :10.1093/mnras/172.3.667 .
^ a b c d Cenarro, A. J.; et al. (January 2007), "Medium-resolution Isaac Newton Telescope library of empirical spectra - II. The stellar atmospheric parameters", Monthly Notices of the Royal Astronomical Society , 374 (2): 664– 690, arXiv :astro-ph/0611618 , Bibcode :2007MNRAS.374..664C , doi :10.1111/j.1365-2966.2006.11196.x , S2CID 119428437 .
^ Famaey, B.; et al. (January 2005), "Local kinematics of K and M giants from CORAVEL/Hipparcos/Tycho-2 data. Revisiting the concept of superclusters", Astronomy and Astrophysics , 430 (1): 165– 186, arXiv :astro-ph/0409579 , Bibcode :2005A&A...430..165F , doi :10.1051/0004-6361:20041272 , S2CID 17804304 .
^ 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 c d van Belle, Gerard T.; von Braun, Kaspar; Ciardi, David R.; Pilyavsky, Genady; Buckingham, Ryan S.; Boden, Andrew F.; Clark, Catherine A.; Hartman, Zachary; van Belle, Gerald; Bucknew, William; Cole, Gary (2021-12-01). "Direct Measurements of Giant Star Effective Temperatures and Linear Radii: Calibration against Spectral Types and V - K Color" . The Astrophysical Journal . 922 (2): 163. arXiv :2107.09205 . Bibcode :2021ApJ...922..163V . doi :10.3847/1538-4357/ac1687 . ISSN 0004-637X . Phi Aurigae's database entry at VizieR .
^ De Medeiros, J. R.; et al. (November 2000), "Rotation and lithium in single giant stars", Astronomy and Astrophysics , 363 : 239– 243, arXiv :astro-ph/0010273 , Bibcode :2000A&A...363..239D .
^ "* phi Aur" . SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 2012-08-23 .
^ van Leeuwen, Floor (November 2007), "Validation of the new Hipparcos reduction", Astronomy and Astrophysics , 474 (2): 653– 664, arXiv :0708.1752v1 , Bibcode :2007A&A...474..653V , doi :10.1051/0004-6361:20078357 , S2CID 18759600 . Note: see VizieR catalogue I/311 .
External links