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41 Aurigae

From Wikipedia, the free encyclopedia
Binary star system in the constellation Auriga
41 Aurigae
Observation data
Epoch J2000      Equinox J2000
ConstellationAuriga
41 Aur A
Right ascension06h 11m 36.59156s[1]
Declination+48° 42′ 39.5603″[1]
Apparent magnitude (V)6.15[2]
41 Aur B
Right ascension06h 11m 36.55589s[3]
Declination+48° 42′ 47.0528″[3]
Apparent magnitude (V)6.84[2]
Characteristics
41 Aur A
Evolutionary stageMain sequence
Spectral typeA2Va+[4]
B−Vcolor index0.06[2]
41 Aur B
Evolutionary stageAm star
Spectral typekA5hA5mF0(IV-V)[4]
B−Vcolor index0.15[2]
Astrometry
41 Aur A
Radial velocity (Rv)31[5] km/s
Proper motion (μ)RA: +15.085[1]mas/yr
Dec.: −55.907[1]mas/yr
Parallax (π)10.5367±0.0689 mas[1]
Distance310 ± 2 ly
(94.9 ± 0.6 pc)
41 Aur B
Radial velocity (Rv)29[5] km/s
Proper motion (μ)RA: +17.183[3] mas/yr
Dec.: −53.536[3] mas/yr
Parallax (π)10.3314 ± 0.0711 mas[3]
Distance316 ± 2 ly
(96.8 ± 0.7 pc)
Details
41 Aur A
Temperature9,000+278
−596
[1] K
Rotational velocity (v sin i)138[6] km/s
41 Aur B
Mass1.99±0.10[7] M
Radius1.78+0.12
−0.18
[3] R
Luminosity11.2±0.1[3] L
Temperature7,925+421
−260
[3] K
Rotational velocity (v sin i)133[7] km/s
Other designations
41 Aur,BD+48°1352,HIP 29388,ADS 4773,WDS J06116+4843
41 Aur A:GC 7853,HD 42127,HR 2176,SAO 40925[8]
41 Aur B:GC 7851,HD 42126,HR 2175,SAO 40924[9]
Database references
SIMBADdata

41 Aurigae is abinary star[10] system located around 310–316 light years away from the Sun in the northernconstellation ofAuriga. It is visible to the naked eye as a dim, white-hued star with a combinedapparent visual magnitude of 5.83.[10] This system is moving further from the Earth with a heliocentricradial velocity of 31 km/s.[11] It is a probable member of theHyades Supercluster.[12]

As of 2012, the pair had anangular separation of7.39 along aposition angle of 357.7°.[13] The primary component is anA-type main-sequence star with astellar classification of A2Va+[4] and a visual magnitude of 6.15.[2] The magnitude 6.84[2] secondary companion is a possibleAm star[14] with astellar classification of kA5hA5mF0(IV-V),[4] showing thecalcium K line andhydrogen lines of anA5 star and themetal lines of anF0 star.

References

[edit]
  1. ^abcdefBrown, 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. ^abcdefHøg, E.; Fabricius, C.; Makarov, V. V.; Urban, S.; Corbin, T.; et al. (March 2000), "The Tycho-2 catalogue of the 2.5 million brightest stars",Astronomy and Astrophysics,355:L27 –L30,Bibcode:2000A&A...355L..27H,doi:10.1888/0333750888/2862.
  3. ^abcdefghBrown, 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.
  4. ^abcdGray, R. O.; Garrison, R. F. (December 1987), "The Early A-Type Stars: Refined MK Classification, Confrontation with Stroemgren Photometry, and the Effects of Rotation",Astrophysical Journal Supplement,65: 581,Bibcode:1987ApJS...65..581G,doi:10.1086/191237.
  5. ^abEvans, D. S. (June 20–24, 1966). "The Revision of the General Catalogue of Radial Velocities". In Batten, Alan Henry; Heard, John Frederick (eds.).Determination of Radial Velocities and their Applications, Proceedings from IAU Symposium no. 30. University of Toronto:International Astronomical Union.Bibcode:1967IAUS...30...57E.
  6. ^Royer, F.; et al. (February 2007), "Rotational velocities of A-type stars. III. Velocity distributions",Astronomy and Astrophysics,463 (2):671–682,arXiv:astro-ph/0610785,Bibcode:2007A&A...463..671R,doi:10.1051/0004-6361:20065224,S2CID 18475298.
  7. ^abZorec, J.; Royer, F. (2012), "Rotational velocities of A-type stars. IV. Evolution of rotational velocities",Astronomy & Astrophysics,537: A120,arXiv:1201.2052,Bibcode:2012A&A...537A.120Z,doi:10.1051/0004-6361/201117691,S2CID 55586789, A120.
  8. ^"41 Aur A".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2019-05-23.
  9. ^"41 Aur B".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2019-05-23.
  10. ^abEggleton, 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.
  11. ^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.
  12. ^Eggen, O. J. (June 1985), "A systematic search for members of the Hyades Supercluster. IV - The metallic-line stars and ultrashort-period Cepheids",Astronomical Journal,90: 1046−1059,Bibcode:1985AJ.....90.1046E,doi:10.1086/113812.
  13. ^Mason, Brian D.; et al. (May 2012), "Speckle Interferometry at the U.S. Naval Observatory. XVIII",The Astronomical Journal,143 (5): 6,Bibcode:2012AJ....143..124M,doi:10.1088/0004-6256/143/5/124, 124.
  14. ^Renson, P.; Manfroid, J. (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.
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