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12 Aurigae

From Wikipedia, the free encyclopedia
Star in the constellation Auriga
12 Aurigae
Observation data
Epoch J2000      Equinox J2000
ConstellationAuriga
Right ascension05h 16m 27.08298s[1]
Declination+46° 24′ 57.8118″[1]
Apparent magnitude (V)6.988[2]
Characteristics
Spectral typeB2 Ve[3]
Astrometry
Proper motion (μ)RA: −3.321[1]mas/yr
Dec.: −1.2106[1]mas/yr
Parallax (π)1.5264±0.0303 mas[1]
Distance2,140 ± 40 ly
(660 ± 10 pc)
Details
Mass3.0[4] M
Radius18[5] R
Luminosity635[5] L
Surface gravity (log g)2.47[4] cgs
Temperature8,688[6] K
Metallicity−0.94[4]
Rotational velocity (v sin i)100±41[7] km/s
Other designations
12 Aur,BD+46°989,GC 6424,HD 33988,SAO 40183,PPM 47919[8]
Database references
SIMBADdata

12 Aurigae is aBe star in the northernconstellationAuriga. It lies below the normal limit for visibility to the naked eye, having anapparent visual magnitude of 6.988.[2] It lacks a designation from theHipparcos catalogue. It is located just under half a degree north ofCapella.[8]

Assignedspectral classes for 12 Aurigae vary greatly from B2 to B5 and theluminosity class from V (main sequence) to Ia (luminoussupergiant). Itsspectrum shows prominentemission lines, but the spectrum is complicated by the appearance of sharpshell components to some of the spectral lines.[9] The colour of the star as shown by the B-V and U-Bcolour indices is not consistent with an early B spectral class,[10] leading to many estimates of itseffective temperature that are much lower than expected for a B-class star.[6][4] The expected temperature for a B5 spectral type would be15,400 K,[11] but most sources assign a temperature of around8,000 K.[6][4] Other properties also vary between different sources, for example thebolometric luminosity derived from the distance and temperature is 25 L,[6] while it is 635 L when derived by fitting thespectral energy distribution.[5] A calculation of the stellar properties assuming the maximum possibleinterstellar extinction in the direction of 12 Aurigae results in a temperature of14,336 K and a luminosity of 8,092 L, although it is strongly noted that the likely extinction is much lower.[5]

References

[edit]
  1. ^abcdeVallenari, A.; et al. (Gaia collaboration) (2023)."Gaia Data Release 3. Summary of the content and survey properties".Astronomy and Astrophysics.674: A1.arXiv:2208.00211.Bibcode:2023A&A...674A...1G.doi:10.1051/0004-6361/202243940.S2CID 244398875. Gaia DR3 record for this source atVizieR.
  2. ^abPaunzen, E. (2015). "A new catalogue of Strömgren-Crawford uvbyβ photometry".Astronomy & Astrophysics.580: A23.arXiv:1506.04568.Bibcode:2015A&A...580A..23P.doi:10.1051/0004-6361/201526413.S2CID 73623700.
  3. ^Burbidge, G. R.; Burbidge, E. Margaret (September 1953)."The Balmer Decrement in Some Be Stars".Astrophysical Journal.118: 252.Bibcode:1953ApJ...118..252B.doi:10.1086/145747.
  4. ^abcdeAnders, F.; Khalatyan, A.; Queiroz, A. B. A.; Chiappini, C.; Ardevol, J.; Casamiquela, L.; Figueras, F.; Jimenez-Arranz, O.; Jordi, C.; Monguio, M.; Romero-Gomez, M.; Altamirano, D.; Antoja, T.; Assaad, R.; Cantat-Gaudin, T.; Castro-Ginard, A.; Enke, H.; Girardi, L.; Guiglion, G.; Khan, S.; Luri, X.; Miglio, A.; Minchev, I.; Ramos, P.; Santiago, B. X.; Steinmetz, M. (2022). "VizieR Online Data Catalog: StarHorse2, Gaia EDR3 photo-astrometric distances (Anders+, 2022)".Vizier Online Data Catalog.Bibcode:2022yCat.1354....0A.
  5. ^abcdMcDonald, I.; Zijlstra, A. A.; Watson, R. A. (15 June 2017)."Fundamental parameters and infrared excesses of Tycho–Gaia stars".Monthly Notices of the Royal Astronomical Society.471 (1):770–791.arXiv:1706.02208.Bibcode:2017MNRAS.471..770M.doi:10.1093/mnras/stx1433.eISSN 1365-2966.ISSN 0035-8711.
  6. ^abcdStassun, Keivan G.; et al. (September 2018)."The TESS Input Catalog and Candidate Target List".The Astronomical Journal.156 (3): 102.arXiv:1706.00495.Bibcode:2018AJ....156..102S.doi:10.3847/1538-3881/aad050.ISSN 0004-6256.
  7. ^Halbedel, Elaine M. (September 1996)."Rotational Velocity Determinations for 164 Be and B Stars".Publications of the Astronomical Society of the Pacific.108: 833.Bibcode:1996PASP..108..833H.doi:10.1086/133804.
  8. ^ab"12 Aur".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2019-04-04.
  9. ^Halbedel, Elaine M. (September 1996)."Rotational Velocity Determinations for 164 Be and B Stars".Publications of the Astronomical Society of the Pacific.108: 833.Bibcode:1996PASP..108..833H.doi:10.1086/133804.S2CID 119944672.
  10. ^Hamdy, M. A.; Elazm, M. S. A.; Saad, S. M. (1991). "Spectral reclassification of some be stars using ΔQ method".Astrophysics and Space Science.186 (1): 161.Bibcode:1991Ap&SS.186..161H.doi:10.1007/BF00644632.S2CID 123509301.
  11. ^Wright, Candace O.; et al. (2003)."The Tycho-2 Spectral Type Catalog".The Astronomical Journal.125 (1): 359.Bibcode:2003AJ....125..359W.doi:10.1086/345511.S2CID 122781581.
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