Star in the constellation Phoenix
λ1 Phoenicis , Latinized as Lambda1 Phoenicis , is a double star [ 10] in the southern constellation of Phoenix . It is visible to the naked eye as a faint, white-hued point of light with a combined apparent visual magnitude of 4.76.[ 2] The system is located approximately 183 light years away from the Sun based on parallax .[ 1] It is a member of the Hyades Supercluster .[ 11]
The brighter component is an A-type main-sequence star with a stellar classification of A0Va.[ 3] It may form a binary system of two roughly equal stars.[ 10] An infrared excess suggests there is a debris disk orbiting 46.3 AU from the star with a mean temperature of 95 K.[ 7] It has one visual companion at an angular separation of about 30″ and magnitude 13.7.[ 12] [ 13]
^ a b c d e f 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 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 . Vizier catalog entry
^ a b Gray, R. O.; Garrison, R. F. (1987). "The Early A-Type Stars: Refined MK Classification, Confrontation with Stroemgren Photometry, and the Effects of Rotation" . The Astrophysical Journal Supplement Series . 65 : 581. Bibcode :1987ApJS...65..581G . doi :10.1086/191237 .
^ a b Mallama, A. (2014). "Sloan Magnitudes for the Brightest Stars". The Journal of the American Association of Variable Star Observers . 42 (2): 443. Bibcode :2014JAVSO..42..443M . Vizier catalog entry
^ Gontcharov, G. A. (2006). "Pulkovo Compilation of Radial Velocities for 35 495 Hipparcos stars in a common system". Astronomy Letters . 32 (11): 759– 771. arXiv :1606.08053 . Bibcode :2006AstL...32..759G . doi :10.1134/S1063773706110065 . S2CID 119231169 .
^ a b c d e David, Trevor J.; Hillenbrand, Lynne A. (2015). "The Ages of Early-Type Stars: Strömgren Photometric Methods Calibrated, Validated, Tested, and Applied to Hosts and Prospective Hosts of Directly Imaged Exoplanets". The Astrophysical Journal . 804 (2): 146. arXiv :1501.03154 . Bibcode :2015ApJ...804..146D . doi :10.1088/0004-637X/804/2/146 . S2CID 33401607 . Vizier catalog entry
^ a b Cotten, Tara H.; Song, Inseok (July 2016). "A Comprehensive Census of Nearby Infrared Excess Stars" . The Astrophysical Journal Supplement Series . 225 (1): 24. arXiv :1606.01134 . Bibcode :2016ApJS..225...15C . doi :10.3847/0067-0049/225/1/15 . S2CID 118438871 . 15.
^ Gontcharov, G. A. (2012). "Dependence of kinematics on the age of stars in the solar neighborhood". Astronomy Letters . 38 (12): 771– 782. arXiv :1606.08814 . Bibcode :2012AstL...38..771G . doi :10.1134/S1063773712120031 . S2CID 118345778 . Vizier catalog entry
^ "lam01 Phe" . SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 2019-09-23 .
^ a b 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 .
^ Eggen, Olin J. (July 1998), "The Age Range of Hyades Stars", The Astronomical Journal , 116 (1): 284– 292, Bibcode :1998AJ....116..284E , doi :10.1086/300413 .
^ Dommanget, J.; Nys, O. (2002). "VizieR Online Data Catalog: CCDM (Catalog of Components of Double & Multiple stars) (Dommanget+ 2002)". VizieR On-line Data Catalog: I/274. Originally Published in: Observations et Travaux 54 . 1274 . Bibcode :2002yCat.1274....0D . Vizier catalog entry
^ Mason, Brian D.; et al. (2001). "The 2001 US Naval Observatory Double Star CD-ROM. I. The Washington Double Star Catalog" . The Astronomical Journal . 122 (6): 3466. Bibcode :2001AJ....122.3466M . doi :10.1086/323920 . Vizier catalog entry