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39 Andromedae

From Wikipedia, the free encyclopedia
Double star in the constellation Andromeda
39 Andromedae
Location of 39 Andromedae (circled)
Observation data
Epoch J2000      Equinox J2000
ConstellationAndromeda
Right ascension01h 02m 54.25356s[1]
Declination+41° 20′ 42.7673″[1]
Apparent magnitude (V)5.95[2]
Characteristics
Spectral typekA3hA7VmA9[3]
B−Vcolor index+0.161±0.009[2]
Astrometry
Radial velocity (Rv)+3.1±0.9[4] km/s
Proper motion (μ)RA: −17.558[1]mas/yr
Dec.: −18.400[1]mas/yr
Parallax (π)9.5725±0.0805 mas[1]
Distance341 ± 3 ly
(104.5 ± 0.9 pc)
Absolute magnitude (MV)0.80[2]
Details
Radius1.2[5] R
Luminosity39.95[2] L
Surface gravity (log g)3.93[6] cgs
Temperature8,073[6] K
Metallicity [Fe/H]+0.13[6] dex
Rotational velocity (v sin i)34[6] km/s
Other designations
39 And,BD+40°209,HD 6116,HIP 4903,HR 290,SAO 36874,PPM 43575,WDS J01029+4121A[7]
Database references
SIMBADdata

39 Andromedae, abbreviated39 And, is adouble star in the northernconstellationAndromeda.39 Andromedae is theFlamsteed designation. Itsapparent visual magnitude is 5.95,[2] which indicates it is near the lower limit on visibility to the naked eye. The distance to this star, as estimated from its annualparallax shift of9.57 mas,[1] is 341 light years. It is a suspected member of theUrsa Major Moving Group, although King et al. (2003) list it as a probable non-member.[8]

The brighter component is a confirmedAm star[9] with astellar classification of kA3hA7VmA9.[3] This notation indicates itsspectrum displays thecalcium K line of an A3 star, thehydrogen lines of an A7 V, orA-type main-sequence star, and themetal lines of an A9 star. It is radiating 40[2] times theSun's luminosity from itsphotosphere at aneffective temperature of 8,073 K.[6] As of 2015, the magnitude 12.48 companion star is located at anangular separation of20.5 along aposition angle of 3° from the primary.[10]

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.
  2. ^abcdefAnderson, 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.
  3. ^abLevato, H.; Abt, H. A. (August 1978), "Spectral types in the Ursa Major stream",Publications of the Astronomical Society of the Pacific,90: 429−433,Bibcode:1978PASP...90..429L,doi:10.1086/130352.
  4. ^de Bruijne, J. H. J.; Eilers, A.-C. (October 2012), "Radial velocities for the HIPPARCOS-Gaia Hundred-Thousand-Proper-Motion project",Astronomy & Astrophysics,546: 14,arXiv:1208.3048,Bibcode:2012A&A...546A..61D,doi:10.1051/0004-6361/201219219,S2CID 59451347, A61.
  5. ^Pasinetti Fracassini, L. E.; et al. (February 2001), "Catalogue of Apparent Diameters and Absolute Radii of Stars (CADARS)",Astronomy and Astrophysics,367 (3rd ed.):521–524,arXiv:astro-ph/0012289,Bibcode:2001A&A...367..521P,doi:10.1051/0004-6361:20000451,S2CID 425754.
  6. ^abcdeMonier, R. (November 2005), "Abundances of a sample of A and F-type dwarf members of the Ursa Major Group",Astronomy and Astrophysics,442 (2):563–566,Bibcode:2005A&A...442..563M,doi:10.1051/0004-6361:20053222.
  7. ^"39 And".SIMBAD.Centre de données astronomiques de Strasbourg. RetrievedSeptember 28, 2018.
  8. ^King, Jeremy R.; et al. (2003), "Stellar Kinematic Groups. II. A Reexamination of the Membership, Activity, and Age of the Ursa Major Group",The Astronomical Journal,125 (4): 1980,Bibcode:2003AJ....125.1980K,doi:10.1086/368241.
  9. ^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.
  10. ^Mason, B. D.; et al. (2014), "The Washington Visual Double Star Catalog",The Astronomical Journal,122 (6): 3466,Bibcode:2001AJ....122.3466M,doi:10.1086/323920

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