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HD 37519

From Wikipedia, the free encyclopedia
Star in the constellation Auriga
HD 37519
Observation data
Epoch J2000      Equinox J2000
ConstellationAuriga
Right ascension05h 40m 35.90737s[1]
Declination+31° 21′ 29.5262″[1]
Apparent magnitude (V)6.04[2]
Characteristics
Spectral typeB9.5III-IV(p)? (Hg?)[3]
U−Bcolor index−0.21[2]
B−Vcolor index+0.05[2]
Variable typesuspected[4]
Astrometry
Radial velocity (Rv)−10.2±3.4[5] km/s
Proper motion (μ)RA: −5.051[1]mas/yr
Dec.: −8.187[1]mas/yr
Parallax (π)4.0335±0.1112 mas[1]
Distance810 ± 20 ly
(248 ± 7 pc)
Absolute magnitude (MV)−0.43[6]
Details
Radius3.0[7] R
Luminosity110[8] L
Temperature8,289[8] K
Rotational velocity (v sin i)195[9] km/s
Age375[6] Myr
Other designations
NSV 2537,BD+31°1048,FK5 2425,HD 37519,HIP 26712,HR 1938,SAO 58319[10]
Database references
SIMBADdata

HD 37519 is astar in the northern constellationAuriga. It has a blue-white hue and is dimly visible to the naked eye with anapparent visual magnitude of 6.04.[2] The distance to HD 37519 is approximately 810 light years based onparallax, but it is drifting closer with aradial velocity of −10 km/s.[5]

Cowley in 1972 found astellar classification of B9.5III-IV(p)? (Hg?) for this star,[3] suggesting it is anevolvedB-type star and a suspectedchemically peculiar star of themercury-manganese type.[11] It is estimated to be 375 million years old and with a high rate of spin, showing aprojected rotational velocity of 195 km/s.[9] In March 1964, a suspected flare of HD 37519 was detected that increased the star's brightness by about three magnitudes. Smaller variations of up to two magnitudes were detected a few days later,[12] suggesting there might be aflare star companion. However, follow-up observations failed to confirm the variability.[13] The star is radiating 110[8] times theluminosity of the Sun from itsphotosphere at aneffective temperature of 8,289 km/s.[8]

References

[edit]
  1. ^abcdeBrown, 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 atVizieR.
  2. ^abcdJohnson, H. L.; et al. (1966), "UBVRIJKL photometry of the bright stars",Communications of the Lunar and Planetary Laboratory,4 (99): 99,Bibcode:1966CoLPL...4...99J.
  3. ^abCowley, A. (November 1972), "Spectral classification of the bright B8 stars",Astronomical Journal,77:750–755,Bibcode:1972AJ.....77..750C,doi:10.1086/111348.
  4. ^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.
  5. ^abGontcharov, G. A. (November 2006), "Pulkovo Compilation of Radial Velocities for 35 495 Hipparcos stars in a common system",Astronomy Letters,32 (11):759–771,arXiv:1606.08053,Bibcode:2006AstL...32..759G,doi:10.1134/S1063773706110065,S2CID 119231169.
  6. ^abGontcharov, G. A. (November 2012), "Spatial distribution and kinematics of OB stars",Astronomy Letters,38 (11):694–706,arXiv:1606.09028,Bibcode:2012AstL...38..694G,doi:10.1134/S1063773712110035,S2CID 119108982.
  7. ^Pasinetti Fracassini, L. E.; et al. (2001), "Catalogue of Apparent Diameters and Absolute Radii of Stars (CADARS) - Third edition - Comments and statistics",Astronomy & Astrophysics,367 (2):521–24,arXiv:astro-ph/0012289,Bibcode:2001A&A...367..521P,doi:10.1051/0004-6361:20000451,S2CID 425754.
  8. ^abcdMcDonald, 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.
  9. ^abAbt, Helmut A.; et al. (July 2002), "Rotational Velocities of B Stars",The Astrophysical Journal,573 (1):359–365,Bibcode:2002ApJ...573..359A,doi:10.1086/340590.
  10. ^"HD 36780".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2019-12-28.
  11. ^Renson, P.; Manfroid, J. (May 2009), "Catalogue of Ap, HgMn and Am stars",Astronomy and Astrophysics,498 (3):961–966,Bibcode:2009A&A...498..961R,doi:10.1051/0004-6361/200810788.
  12. ^Mammano, A. (May 1966), "Spectrum of the Early-Type Flare Star BD +13 1048",Information Bulletin on Variable Stars,134: 1,Bibcode:1966IBVS..134....1M.
  13. ^Andrews, A. D. (July 1996), "A Re-Examination of the Suspected Early-Type Flare Star BD+31 1048 (bs 1938) in Auriga: a Skeleton from the Cupboard",Irish Astronomical Journal,23 (2): 189,Bibcode:1996IrAJ...23..189A.

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