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Link to original content: http://en.wikipedia.org/wiki/V372_Carinae
V372 Carinae - Wikipedia Jump to content

V372 Carinae

From Wikipedia, the free encyclopedia
V372 Carinae

A light curve for V372 Carinae, plotted from TESS data[1]
Observation data
Epoch J2000      Equinox J2000
Constellation Carina
Right ascension 07h 52m 29.74145s[2]
Declination −54° 22′ 01.7898″[2]
Apparent magnitude (V) 5.70[3]
Characteristics
Spectral type B1.5IV
B−V color index −0.151±0.004[3]
Variable type Beta Cephei[4]
Astrometry
Radial velocity (Rv)+18.0±4.3[3] km/s
Proper motion (μ) RA: −4.534[2] mas/yr
Dec.: +8.642[2] mas/yr
Parallax (π)2.3134 ± 0.1239 mas[2]
Distance1,410 ± 80 ly
(430 ± 20 pc)
Absolute magnitude (MV)−2.35[3]
Details
Mass10.1±0.1[5] M
Radius8.4[6] R
Luminosity1,742[7] L
Temperature14,132[7] K
Age15.8±2.2[5] Myr
Other designations
V372 Car, CD−54°1966, HD 64722, HIP 38438, HR 3088, SAO 235579[8]
Database references
SIMBADdata

V372 Carinae is a single[9] star in the southern constellation of Carina. Located around 1300 light-years distant. It shines with a luminosity approximately 1742 times that of the Sun and has a surface temperature of 14132 K.[7] It is a Beta Cephei variable.[4]

References

[edit]
  1. ^ "MAST: Barbara A. Mikulski Archive for Space Telescopes". Space Telescope Science Institute. Retrieved 8 December 2021.
  2. ^ a b c d e 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. ^ 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.
  4. ^ a b Dubath, P.; Rimoldini, L.; Süveges, M.; Blomme, J.; López, M.; Sarro, L. M.; et al. (2011). "Random forest automated supervised classification of Hipparcos periodic variable stars". Monthly Notices of the Royal Astronomical Society. 414 (3): 2602–17. arXiv:1101.2406. Bibcode:2011MNRAS.414.2602D. doi:10.1111/j.1365-2966.2011.18575.x. S2CID 118560311.
  5. ^ a b 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.
  6. ^ Pasinetti Fracassini, L. E.; et al. (2001). "Catalogue of Apparent Diameters and Absolute Radii of Stars (CADARS)". Astronomy & Astrophysics. 367 (Third ed.): 521–24. arXiv:astro-ph/0012289. Bibcode:2001A&A...367..521P. doi:10.1051/0004-6361:20000451. S2CID 425754.
  7. ^ a b c McDonald, I.; et al. (2012). "Fundamental Parameters and Infrared Excesses of Hipparcos Stars". Monthly Notices of the Royal Astronomical Society. 427 (1): 343–57. arXiv:1208.2037. Bibcode:2012MNRAS.427..343M. doi:10.1111/j.1365-2966.2012.21873.x. S2CID 118665352.
  8. ^ "V372 Car". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2020-02-18.
  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.