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59 Aurigae

From Wikipedia, the free encyclopedia
Star in the constellation Auriga
59 Aurigae

Fourvisual bandlight curves for 59 Aurigae, adapted from Zhiping (2000)[1]
Observation data
Epoch J2000      Equinox J2000
ConstellationAuriga
Right ascension06h 53m 01.41099s[2]
Declination+38° 52′ 08.9353″[2]
Apparent magnitude (V)6.099[3]
Characteristics
Spectral typeF2V[4]
U−Bcolor index+0.14[5]
B−Vcolor index+0.38[5]
Variable typeδ Sct[6]
Astrometry
Radial velocity (Rv)1.0±4.3[7] km/s
Proper motion (μ)RA: −3.935[2]mas/yr
Dec.: 6.454[2]mas/yr
Parallax (π)6.7493±0.0501 mas[2]
Distance483 ± 4 ly
(148 ± 1 pc)
Absolute magnitude (MV)0.23±0.12[8]
Details
Mass2.49±0.08[9] M
Radius5.73+0.29
−0.26
[2] R
Luminosity63.87±0.65[2] L
Temperature6,808[8] K
Metallicity[Fe/H]0.18[8] dex
Rotational velocity (v sin i)165[9] km/s
Age700±100[8] Myr
Other designations
59 Aur,OX Aur,BD+39°1771,GC 8993,HD 50018,HIP 33041,HR 2539,SAO 59571,PPM 72197,ADS 5534,CCDM J06530+3852,WDS J06530+3852,TYC 2942-2005-1,GSC 02942-02005
Database references
SIMBADdata

59 Aurigae, often abbreviated as59 Aur, is astar in theconstellationAuriga. Its baselineapparent magnitude is 6.1,[3] meaning it can just barely be seen with thenaked eye as a dim, yellow-white hued star. Based onparallax measurements, it is located about 483light-years (148parsecs) away from the Sun.[2]

In 1966, Ivan John Danziger and Robert John Dickens discovered that 59 Aurigae star is avariable star.[10] This object is aDelta Scuti variable, meaning it varies in luminosity due to pulsations on its surface, ranging in magnitude from 5.94 down to 6.14 with a period of 0.154412 days (3.7 h).[6] For that reason, in 1975, it was given thevariable star designationOX Aurigae.[11] The star'sspectrum matches that of anF-type main-sequence star and it has aspectral type of F2V.[4] It has 2.5[9] times themass of the Sun and 5.7[2] times the Sun's radius. 59 Aurigae is thought to be around 700 million years old, and is radiating 64[2] times theSun's luminosity from itsphotosphere aneffective temperature of 6,808 K.[8]

References

[edit]
  1. ^Zhiping, Li (October 2000)."Complicated pulsation in the delta Scuti variable 59 Aurigae".Astronomy and Astrophysics.362:595–598.Bibcode:2000A&A...362..595L. Retrieved31 October 2021.
  2. ^abcdefghijBrown, 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.
  3. ^abHøg, E.; et al. (2000). "The Tycho-2 catalogue of the 2.5 million brightest stars".Astronomy and Astrophysics.355:L27 –L30.Bibcode:2000A&A...355L..27H.
  4. ^abAbt, Helmut A.; Morrell, Nidia I. (1995)."The Relation between Rotational Velocities and Spectral Peculiarities among A-Type Stars".Astrophysical Journal Supplement.99: 135.Bibcode:1995ApJS...99..135A.doi:10.1086/192182.
  5. ^abMermilliod, J.-C. (1986). "Compilation of Eggen's UBV data, transformed to UBV (unpublished)".Catalogue of Eggen's UBV Data.Bibcode:1986EgUBV........0M.
  6. ^abSamus, 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.
  7. ^Gontcharov, G. A. (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.
  8. ^abcdeNordström, B.; et al. (2004). "The Geneva-Copenhagen survey of the Solar neighbourhood. Ages, metallicities, and kinematic properties of ˜14 000 F and G dwarfs".Astronomy and Astrophysics.418:989–1019.arXiv:astro-ph/0405198.Bibcode:2004A&A...418..989N.doi:10.1051/0004-6361:20035959.S2CID 11027621.
  9. ^abcZorec, 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.
  10. ^Danziger, I. J.; Dickens, R. J. (August 1966)."Observations of Variable F-Type Stars with Short Periods"(PDF).Information Bulletin on Variable Stars.150.Bibcode:1966IBVS..150....1D. Retrieved29 November 2024.
  11. ^Kukarkin, B. V.; Kholopov, P. N.; Kukarkina, N. P. (November 1975)."61st Name-List of Variable Stars"(PDF).Information Bulletin on Variable Stars.1068:1–5.Bibcode:1975IBVS.1068....1K. Retrieved30 November 2024.

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