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HD 83183

From Wikipedia, the free encyclopedia
This article is about h Carinae. For H Carinae, see HD 83095.
HD 83183
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Carina
Right ascension 09h 34m 26.65081s[1]
Declination −59° 13′ 47.1070″[1]
Apparent magnitude (V) 4.08[2]
Characteristics
Spectral type B5 II[3]
B−V color index −0.013±0.003[2]
Astrometry
Radial velocity (Rv)+18.2±0.6[2] km/s
Proper motion (μ) RA: −10.74[1] mas/yr
Dec.: +6.60[1] mas/yr
Parallax (π)2.46 ± 0.10 mas[1]
Distance1,330 ± 50 ly
(410 ± 20 pc)
Absolute magnitude (MV)−3.96[2]
Details
Mass9.4±0.5[4] M☉
Radius18[5] R☉
Luminosity11,634[6] L☉
Surface gravity (log g)2.50[7] cgs
Temperature14,300[6] K
Rotational velocity (v sin i)19±4[7] km/s
Age24.5±3.8[4] Myr
Other designations
h Car, CPD−58°1576, GC 13246, HD 83183, HIP 46974, HR 3825, SAO 237117[8]
Database references
SIMBADdata

HD 83183 is a single[9] star in the southern constellation of Carina. It has the Bayer designation h Carinae, while HD 83183 is the star's identifier from the Henry Draper catalogue. The star is blue-white in hue and is faintly visible to the naked eye with an apparent visual magnitude of 4.08.[2] It is located at a distance of approximately 1,330 light years based on parallax,[1] and is drifting further away with a radial velocity of +18 km/s.[2] O. J. Eggen identified it as a member of the Pleiades group of co-moving stars.[10]

This object is a massive bright giant star with a stellar classification of B5 II.[3] It is 25[4] million years old and is spinning with a projected rotational velocity of 19 km/s.[7] The star has 9[4] times the mass of the Sun and about 18[5] times the Sun's radius. It is radiating 11,634 times the luminosity of the Sun from its enlarged photosphere at an effective temperature of 14,300 K.[6]

References

[edit]
  1. ^ a b c d e f van Leeuwen, F. (2007), "Validation of the new Hipparcos reduction", Astronomy and Astrophysics, 474 (2): 653–664, arXiv:0708.1752, Bibcode:2007A&A...474..653V, doi:10.1051/0004-6361:20078357.
  2. ^ a b c d e f 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
  3. ^ a b Houk, Nancy; Cowley, A. P. (1979), Michigan catalogue of two-dimensional spectral types for the HD stars, vol. 1, Ann Arbor, Michigan: Dept. of Astronomy, University of Michigan, Bibcode:1978mcts.book.....H
  4. ^ a b c d 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.
  5. ^ a b Pasinetti Fracassini, L. E.; et al. (2001), "Catalogue of Apparent Diameters and Absolute Radii of Stars (CADARS)", Astronomy & Astrophysics, 367 (2) (Third ed.): 521–24, arXiv:astro-ph/0012289, Bibcode:2001A&A...367..521P, doi:10.1051/0004-6361:20000451, S2CID 425754.
  6. ^ a b c Hohle, M. M.; et al. (2010), "Masses and luminosities of O- and B-type stars and red supergiants", Astronomische Nachrichten, 331 (4): 349–360, arXiv:1003.2335, Bibcode:2010AN....331..349H, doi:10.1002/asna.200911355, S2CID 111387483.
  7. ^ a b c Fraser, M.; Dufton, P. L.; Hunter, I.; Ryans, R. S. I. (2010), "Atmospheric parameters and rotational velocities for a sample of Galactic B-type supergiants", Monthly Notices of the Royal Astronomical Society, 404 (3): 1306, arXiv:1001.3337, Bibcode:2010MNRAS.404.1306F, doi:10.1111/j.1365-2966.2010.16392.x, S2CID 118674151.
  8. ^ "HD 83183". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2020-01-26.
  9. ^ 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.
  10. ^ Eggen, O. J. (February 1974), "NGC 2287 and the Pleiades group", Astrophysical Journal, 188: 59–70, Bibcode:1974ApJ...188...59E, doi:10.1086/152685.
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