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Xi Aurigae

From Wikipedia, the free encyclopedia
Star in the constellation Auriga
Xi Aurigae
Observation data
EpochJ2000.0      EquinoxJ2000.0 (ICRS)
ConstellationAuriga
Right ascension05h 54m 50.76694s[1]
Declination+55° 42′ 25.0802″[1]
Apparent magnitude (V)+5.00[2]
Characteristics
Spectral typeA2 Va[3]
U−Bcolor index+0.12[2]
B−Vcolor index+0.05[2]
Astrometry
Radial velocity (Rv)−13.3±2.4[4] km/s
Proper motion (μ)RA: −7.049[1]mas/yr
Dec.: +12.959[1]mas/yr
Parallax (π)13.3702±0.1670 mas[1]
Distance244 ± 3 ly
(74.8 ± 0.9 pc)
Absolute magnitude (MV)+0.64[5]
Details[6]
Mass1.96 M
Radius1.1[7] R
Luminosity49.5[5] L
Surface gravity (log g)3.88 cgs
Temperature9,152±311 K
Metallicity [Fe/H]−0.36±0.04[5] dex
Rotational velocity (v sin i)62 km/s
Age174 Myr
Other designations
ξ Ari,30 Aurigae,BD+55° 1027,FK5 1157,HD 39283,HIP 27949,HR 2029,SAO 25450[8]
Database references
SIMBADdata

Xi Aurigae,Latinized from ξ Aurigae, is theBayer designation for a single,[9] white-huedstar in the northernconstellation ofAuriga. This star was once considered part of the constellation ofCamelopardalis and held theFlamsteed designation32 Camelopardalis.[10] It is visible to the naked eye with anapparent visual magnitude of +5.0.[2] The measured annualparallax shift of this star is13.37 ± 0.17mas,[1] which corresponds to a physical distance of 244light-years (75parsecs) with a 3 light-yearmargin of error. At that distance, the visual magnitude of the star is diminished by anextinction of 0.108 due tointerstellar dust.[11]

This is anA-type main sequence star with astellar classification of A2 Va.[3] Although it was one of the first stars to be cataloged as aLambda Boötis star, Murphy et al. (2015) don't consider it to be a member of this population.[3] The star has nearly twice[6] themass of the Sun and about 1.1[7] times theSun's radius. It is an estimated 174[6] million years old and is spinning with aprojected rotational velocity of 62 km/s.[6] Xi Aurigae is radiating 49.5[5] times theSun's luminosity from itsphotosphere at aneffective temperature of around 9,152 K.[6]

References

[edit]
  1. ^abcdefVallenari, 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. ^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. ^abcMurphy, Simon J.; et al. (October 2015), "An Evaluation of the Membership Probability of 212 λ Boo Stars. I. A Catalogue",Publications of the Astronomical Society of Australia,32: 43,arXiv:1508.03633,Bibcode:2015PASA...32...36M,doi:10.1017/pasa.2015.34,S2CID 59405545, e036.
  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. ^abcdAnderson, 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.
  6. ^abcdeDavid, Trevor J.; Hillenbrand, Lynne A. (2015), "The Ages of Early-Type Stars: Strömgren Photometric Methods Calibrated, Validated, Tested, and Applied to Hosts and Prospective Hosts of Directly Imaged Exoplanets",The Astrophysical Journal,804 (2): 146,arXiv:1501.03154,Bibcode:2015ApJ...804..146D,doi:10.1088/0004-637X/804/2/146,S2CID 33401607.
  7. ^abPasinetti Fracassini, L. E.; et al. (February 2001), "Catalogue of Apparent Diameters and Absolute Radii of Stars (CADARS)",Astronomy and Astrophysics,367 (Third ed.):5211–524,arXiv:astro-ph/0012289,Bibcode:2001A&A...367..521P,doi:10.1051/0004-6361:20000451,S2CID 425754.
  8. ^"ksi Aur".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2017-09-28.
  9. ^Eggleton, P. P.; Tokovinin, A. A. (2008), "A catalogue of multiplicity among bright stellar systems",Monthly Notices of the Royal Astronomical Society,389 (2): 869,arXiv:0806.2878,Bibcode:2008MNRAS.389..869E,doi:10.1111/j.1365-2966.2008.13596.x,S2CID 14878976.
  10. ^Wagman, M. (August 1987), "Flamsteed's Missing Stars",Journal for the History of Astronomy,18 (3): 213,Bibcode:1987JHA....18..209W,doi:10.1177/002182868701800305,S2CID 118445625.
  11. ^Murphy, Simon J.; Paunzen, Ernst (April 2017), "Gaia's view of the λ Boo star puzzle",Monthly Notices of the Royal Astronomical Society,466 (1):546–555,arXiv:1612.01528,Bibcode:2017MNRAS.466..546M,doi:10.1093/mnras/stw3141,S2CID 119328659.

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