Astronomy:HD 83058

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Short description: Binary star system in the constellation Vela
HD 83058
Observation data
Equinox J2000.0]] (ICRS)
Constellation Vela
Right ascension  09h 34m 08.793s[1]
Declination −51° 15′ 18.95″[1]
Apparent magnitude (V) 5.00[2]
Characteristics
Evolutionary stage subgiant
Spectral type B2 IV[3]
U−B color index −0.97[2]
B−V color index −0.19[2]
Astrometry
Radial velocity (Rv)+16.5±3.0[4] km/s
Proper motion (μ) RA: −130.55[1] mas/yr
Dec.: +42.98[1] mas/yr
Parallax (π)3.4252 ± 0.1907[1] mas
Distance950 ± 50 ly
(290 ± 20 pc)
Absolute magnitude (MV)−2.84[2]
Details
primary
Mass9.3[5] M
Radius5.405[6] R
Luminosity2,686[6] L
Surface gravity (log g)3.779[6] cgs
Temperature17,887[6] K
Rotational velocity (v sin i)64±2[4] km/s
Age14.1[5] Myr
secondary
Rotational velocity (v sin i)24±2[4] km/s
Other designations
L Vel, CD−50°4270, FK5 2764, HD 83058, HIP 46950, HR 3819, SAO 237107[7]
Database references
SIMBADdata

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,[8] but high-resolution spectra show it to be a double-lined spectroscopic binary.[9] The two components have approximately the same spectral type.[4] Line-profile variations have been detected which suggest that at least one component pulsates, as is common for stars of this spectral class.[10]

HD 83058 was proposed as a runaway star from a supernova explosion. However, the discovery that it was a binary make this unlikely.[4]

References

  1. 1.0 1.1 1.2 1.3 1.4 Brown, A. G. A. (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics 616: A1. doi:10.1051/0004-6361/201833051. Bibcode2018A&A...616A...1G.  Gaia DR2 record for this source at VizieR.
  2. 2.0 2.1 2.2 2.3 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. doi:10.1007/s10509-020-03827-0. Bibcode2020Ap&SS.365..112M. 
  3. Houk, Nancy (1978). Michigan catalogue of two-dimensional spectral types for the HD stars. Bibcode1978mcts.book.....H. 
  4. 4.0 4.1 4.2 4.3 4.4 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. doi:10.1088/0004-637X/721/1/469. Bibcode2010ApJ...721..469J. 
  5. 5.0 5.1 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. doi:10.1111/j.1365-2966.2010.17434.x. Bibcode2011MNRAS.410..190T. 
  6. 6.0 6.1 6.2 6.3 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. doi:10.1093/mnras/stx1433. Bibcode2017MNRAS.471..770M. 
  7. "HD 83058". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=HD+83058. 
  8. 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. doi:10.1111/j.1365-2966.2008.13596.x. Bibcode2008MNRAS.389..869E. 
  9. 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. doi:10.1111/j.1365-2966.2012.21317.x. Bibcode2012MNRAS.424.1925C. 
  10. 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. doi:10.1051/0004-6361:20054730. Bibcode2006A&A...452..945T.