HD 83058
Binary star system in the constellation Vela
This article is about L Velorum. For l Velorum, see
HD 79917 .
HD 83058 is a subgiant star in the constellation Vela and a spectroscopic binary . It is visible to the naked eye with an apparent visual magnitude of 5.0. Based upon an annual parallax shift of 3.4254 mas , it is located 950 light-years from the Sun . The system is moving further away with a heliocentric radial velocity of + 35 km/s .
HD 83058 has generally been considered to be a single star, but high-resolution spectra show it to be a double-lined spectroscopic binary . The two components have approximately the same spectral type . Line-profile variations have been detected which suggest that at least one component pulsates, as is common for stars of this spectral class.
HD 83058 was proposed as a runaway star from a supernova explosion. However, the discovery that it is a binary makes this unlikely.
References
↑ Roman, Nancy G. (1987). "Identification of a constellation from a position" . Publications of the Astronomical Society of the Pacific . 99 (617): 695. Bibcode :1987PASP...99..695R . doi :10.1086/132034 .
Constellation record for this object at VizieR .
1 2 3 4 5 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 .
1 2 3 4 Melnik, A. M.; Dambis, A. K. (2020). "Distance scale for high-luminosity stars in OB associations and in field with Gaia DR2. Spurious systematic motions". Astrophysics and Space Science . 365 (7): 112. arXiv :2006.14649 . Bibcode :2020Ap& SS.365..112M . doi :10.1007/s10509-020-03827-0 . S2CID 220128144 .
↑ Houk, Nancy (1978). Michigan catalogue of two-dimensional spectral types for the HD stars . Bibcode :1978mcts.book.....H .
1 2 3 4 5 Jilinski, E.; Ortega, V. G.; Drake, N. A.; de la Reza, R. (2010). "A Dynamical Study of Suspected Runaway Stars as Traces of Past Supernova Explosions in the Region of the Scorpius-Centaurus OB Association". The Astrophysical Journal . 721 (1): 469. Bibcode :2010ApJ...721..469J . doi :10.1088/0004-637X/721/1/469 . S2CID 122201360 .
1 2 Tetzlaff, N.; Neuhäuser, R.; Hohle, M. M. (2011). "A catalogue of young runaway Hipparcos stars within 3 KPC from the Sun" . Monthly Notices of the Royal Astronomical Society . 410 (1): 190. arXiv :1007.4883 . Bibcode :2011MNRAS.410..190T . doi :10.1111/j.1365-2966.2010.17434.x . S2CID 118629873 .
1 2 3 4 McDonald, I.; Zijlstra, A. A.; Watson, R. A. (2017). "Fundamental parameters and infrared excesses of Tycho-Gaia stars" . Monthly Notices of the Royal Astronomical Society . 471 (1): 770. arXiv :1706.02208 . Bibcode :2017MNRAS.471..770M . doi :10.1093/mnras/stx1433 . S2CID 73594365 .
↑ "HD 83058" . SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 2020-10-07 .
↑ Eggleton, P. P.; Tokovinin, A. A. (2008). "A catalogue of multiplicity among bright stellar systems" . Monthly Notices of the Royal Astronomical Society . 389 (2): 869. arXiv :0806.2878 . Bibcode :2008MNRAS.389..869E . doi :10.1111/j.1365-2966.2008.13596.x . S2CID 14878976 .
↑ Chini, R.; Hoffmeister, V. H.; Nasseri, A.; Stahl, O.; Zinnecker, H. (2012). "A spectroscopic survey on the multiplicity of high-mass stars" . Monthly Notices of the Royal Astronomical Society . 424 (3): 1925. arXiv :1205.5238 . Bibcode :2012MNRAS.424.1925C . doi :10.1111/j.1365-2966.2012.21317.x . S2CID 119120749 .
↑ Telting, J. H.; Schrijvers, C.; Ilyin, I. V.; Uytterhoeven, K.; De Ridder, J.; Aerts, C.; Henrichs, H. F. (2006). "A high-resolution spectroscopy survey of β Cephei pulsations in bright stars" . Astronomy and Astrophysics . 452 (3): 945. Bibcode :2006A& A...452..945T . doi :10.1051/0004-6361:20054730 . hdl :2066/36162 .