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V376 Carinae

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(Redirected from B1 Carinae) Star in the constellation Carina This article is about b Carinae. For b Carinae, see HD 77370. For B Carinae, see HR 3220. Not to be confused with β Carinae.
V376 Carinae

A light curve for V376 Carinae, plotted from TESS data
Observation data
Epoch J2000      Equinox J2000
Constellation Carina
Right ascension 08 56 58.41666
Declination −59° 13′ 45.6032″
Apparent magnitude (V) 4.69 (4.87 + 6.58)
Characteristics
Spectral type B2V + B9.5V
B−V color index −0.182±0.004
Astrometry
Radial velocity (Rv)+26.8±2.8 km/s
Proper motion (μ) RA: −8.409±0.406 mas/yr
Dec.: +8.421±0.322 mas/yr
Parallax (π)5.0495 ± 0.1667 mas
Distance650 ± 20 ly
(198 ± 7 pc)
Absolute magnitude (MV)−1.64
Details
A
Mass7.8±0.1 M
Luminosity (bolometric)2,998 L
Temperature21,150 K
Age12.5±1.6 Myr
Other designations
b Car, V376 Carinae, CD−58°1301, FK5 1233, GC 12405, HD 77002, HIP 43937, HR 3582, SAO 236436, CCDM J08570-5914, WDS J08570-5914
Database references
SIMBADdata

V376 Carinae is a binary star system in the southern constellation of Carina. It has the Bayer designation b Carinae; V376 Carinae is the variable star designation. The system is visible to the naked eye as a faint point of light with a combined apparent magnitude of +4.69. The distance to this system from the Sun is approximately 650 light years based on parallax. It is drifting further away with a radial velocity of +27 km/s.

The magnitude 4.87 primary, designated component A, is a B-type main-sequence star with a stellar classification of B2V. During a search for Beta Cephei variables in the southern sky, it was initially classed as a very short period variable. However, this variability was not confirmed by subsequent observations. Samus et al. (2017) now suspect it is a constant star that was assigned a variable designation in haste. It has an estimated age of 12.5 million years with 7.8 times the mass of the Sun. The star is radiating nearly three thousand times the Sun's luminosity from its photosphere at an effective temperature of 21,150 K.

The companion star, component B, was discovered by Scottish astronomer James Dunlop in 1836. It has a class of B9.5V with an apparent magnitude of +6.58. As of 2010, the secondary had an angular separation of 40.1 from the primary along a position angle of 76°.

References

  1. "MAST: Barbara A. Mikulski Archive for Space Telescopes". Space Telescope Science Institute. Retrieved 8 December 2021.
  2. ^ 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.
  3. ^ 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.
  4. ^ Mason, B. D.; et al. (2014). "The Washington Visual Double Star Catalog". The Astronomical Journal. 122 (6): 3466–3471. Bibcode:2001AJ....122.3466M. doi:10.1086/323920.
  5. ^ Houk, Nancy (1979). Michigan catalogue of two-dimensional spectral types for the HD stars. Vol. 1. Ann Arbor, Michigan: Department of Astronomy, University of Michigan. Bibcode:1978mcts.book.....H.
  6. ^ 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.
  7. ^ Tetzlaff, N.; et al. (January 2011). "A catalogue of young runaway Hipparcos stars within 3 kpc from the Sun". Monthly Notices of the Royal Astronomical Society. 410 (1): 190–200. arXiv:1007.4883. Bibcode:2011MNRAS.410..190T. doi:10.1111/j.1365-2966.2010.17434.x. S2CID 118629873.
  8. ^ Hohle, M. M.; et al. (April 2010), "Masses and luminosities of O- and B-type stars and red supergiants", Astronomische Nachrichten, 331 (4): 349, arXiv:1003.2335, Bibcode:2010AN....331..349H, doi:10.1002/asna.200911355, S2CID 111387483
  9. "HD 77002". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2020-08-08.
  10. Jakate, S. M. (April 1979). "A search for Beta Cephei stars. III. Photometric studies of southern B-type stars". Astronomical Journal. 84: 552–558. Bibcode:1979AJ.....84..552J. doi:10.1086/112448.
  11. Balona, L. A. (March 1982). "Observations of Early-Type Ultra-Short Period Variables". Information Bulletin on Variable Stars. 2120: 1. Bibcode:1982IBVS.2120....1B.
  12. Samus, N. N.; et al. (2017). "General Catalogue of Variable Stars". Astronomy Reports. 5.1. 61 (1): 80–88. Bibcode:2017ARep...61...80S. doi:10.1134/S1063772917010085. S2CID 125853869.
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