BI 253

BI 253

NW portion of the Tarantula Nebula, with BI 253 towards the top right
Credit: Hubble Legacy Archive
Observation data
Epoch J2000      Equinox J2000
Constellation Dorado
Right ascension 05h 37m 34.461s[1]
Declination −69° 01′ 10.20″[1]
Apparent magnitude (V) 13.76[2]
Characteristics
Evolutionary stage Main sequence[3]
Spectral type O2V-III(n)((f*))[3]
U−B color index −1.02[4]
B−V color index −0.13[4]
Astrometry
Proper motion (μ) RA: 2.3[1] mas/yr
Dec.: 3.1[1] mas/yr
Distance164,000 ly
(50,000[5] pc)
Absolute magnitude (MV)−5.7[3]
Details[6]
Mass97.6 M
Radius13.9 R
Luminosity1,175,000 L
Surface gravity (log g)4.02 cgs
Temperature54,000 K
Rotational velocity (v sin i)185 km/s
Age0.4+0.8
−0.4
 Myr
Other designations
BI 253, VFTS 72, 2MASS J05373446-6901102, IRSF J05373446-6901102
Database references
SIMBADdata

BI 253 is an O2V star in the Large Magellanic Cloud and is a primary standard of the O2 type. It is one of the hottest main-sequence stars known and one of the most-massive and most-luminous stars known.

  1. ^ a b c d Zacharias, N.; Urban, S. E.; Zacharias, M. I.; Wycoff, G. L.; Hall, D. M.; Germain, M. E.; Holdenried, E. R.; Winter, L. (2003). "VizieR Online Data Catalog: The Second U.S. Naval Observatory CCD Astrograph Catalog (UCAC2)". CDS/ADC Collection of Electronic Catalogues. 1289. Bibcode:2003yCat.1289....0Z.
  2. ^ Rivero González, J. G.; Puls, J.; Najarro, F.; Brott, I. (2012). "Nitrogen line spectroscopy of O-stars. II. Surface nitrogen abundances for O-stars in the Large Magellanic Cloud". Astronomy & Astrophysics. 537: A79. arXiv:1110.5148. Bibcode:2012A&A...537A..79R. doi:10.1051/0004-6361/201117790. S2CID 119110554.
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  4. ^ a b Cite error: The named reference bi was invoked but never defined (see the help page).
  5. ^ Evans, C. J.; Taylor, W. D.; Hénault-Brunet, V.; Sana, H.; De Koter, A.; Simón-Díaz, S.; Carraro, G.; Bagnoli, T.; Bastian, N.; Bestenlehner, J. M.; Bonanos, A. Z.; Bressert, E.; Brott, I.; Campbell, M. A.; Cantiello, M.; Clark, J. S.; Costa, E.; Crowther, P. A.; De Mink, S. E.; Doran, E.; Dufton, P. L.; Dunstall, P. R.; Friedrich, K.; Garcia, M.; Gieles, M.; Gräfener, G.; Herrero, A.; Howarth, I. D.; Izzard, R. G.; et al. (2011). "The VLT-FLAMES Tarantula Survey. I. Introduction and observational overview". Astronomy & Astrophysics. 530: A108. arXiv:1103.5386. Bibcode:2011A&A...530A.108E. doi:10.1051/0004-6361/201116782. S2CID 54501763.
  6. ^ Schneider, F. R. N.; Sana, H.; Evans, C. J.; Bestenlehner, J. M.; Castro, N.; Fossati, L.; Gräfener, G.; Langer, N.; Ramírez-Agudelo, O. H.; Sabín-Sanjulián, C.; Simón-Díaz, S.; Tramper, F.; Crowther, P. A.; De Koter, A.; De Mink, S. E.; Dufton, P. L.; Garcia, M.; Gieles, M.; Hénault-Brunet, V.; Herrero, A.; Izzard, R. G.; Kalari, V.; Lennon, D. J.; Maíz Apellániz, J.; Markova, N.; Najarro, F.; Podsiadlowski, Ph.; Puls, J.; Taylor, W. D.; et al. (2018). "An excess of massive stars in the local 30 Doradus starburst". Science. 359 (6371): 69–71. arXiv:1801.03107. Bibcode:2018Sci...359...69S. doi:10.1126/science.aan0106. PMID 29302009. S2CID 206658504.