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40 Persei

From Wikipedia, the free encyclopedia
Star in the constellation Perseus
This article is about o Persei; it is not to be confused withο (omicron) Persei.
40 Persei
Location of 40 Persei (circled)
Observation data
Epoch J2000      Equinox J2000
ConstellationPerseus
Right ascension03h 42m 22.64555s[1]
Declination+33° 57′ 54.0893″[1]
Apparent magnitude (V)4.97[2]
Characteristics
Spectral typeB0.5V[3] + A1Vn[4]
U−Bcolor index−0.84[5]
B−Vcolor index+0.00[5]
Astrometry
Radial velocity (Rv)+22.00[6] km/s
Proper motion (μ)RA: +2.71[1]mas/yr
Dec.: −5.91[1]mas/yr
Parallax (π)3.09±0.21 mas[1]
Distance1,060 ± 70 ly
(320 ± 20 pc)
Absolute magnitude (MV)−2.26[2]
Details
40 Per A
Mass12.5[7] M
Luminosity936[2] L
Surface gravity (log g)4.36[8] cgs
Temperature29,330[9] K
Metallicity[Fe/H]−0.43[2] dex
Rotational velocity (v sin i)10[10] km/s
Age7.2[11] Myr
Other designations
40 Per,BD+33°698,GC 4420,HD 22951,HIP 17313,HR 1123,SAO 56646,CCDM J03424+3358A,WDS J03424+3358A[12]
Database references
SIMBADdata

40 Persei is a widebinary star[13] system in the northernconstellation ofPerseus. It has theBayer designationο Persei, while40 Persei is theFlamsteed designation. The system is visible to the naked eye as a faint, blue-white hued point of light with anapparent visual magnitude of 4.97.[2] It is located approximately 1060 light years away from the Sun based onparallax,[1] and is drifting further away with aradial velocity of +22 km/s.[6] The system is a member of the Perseus OB2 association of co-moving stars.[14]

The primary component is a massiveB-type main-sequence star with astellar classification of B0.5V.[3] It is about 7.2[11] million years old and has a very lowprojected rotational velocity for anearly B-type star,[15] measured at 10 km/s.[10] This star has 12.5[7] times themass of the Sun and is radiating 936[2] times theSun's luminosity from itsphotosphere at aneffective temperature of 29,330 K.[9] The companion is magnitude 10.04,A-type main-sequence star with a class of A1Vn, and is located at anangular separation of19.8 from the primary.[4]

References

[edit]
  1. ^abcdefVan Leeuwen, F. (2007). "Validation of the new Hipparcos reduction".Astronomy and Astrophysics.474 (2):653–664.arXiv:0708.1752.Bibcode:2007A&A...474..653V.doi:10.1051/0004-6361:20078357.S2CID 18759600.Vizier catalog entry
  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.Vizier catalog entry
  3. ^abHoffleit, D.; Warren, W. H. (1995). "VizieR Online Data Catalog: Bright Star Catalogue, 5th Revised Ed. (Hoffleit+, 1991)".VizieR On-line Data Catalog: V/50. Originally Published in: 1964BS....C......0H.5050.Bibcode:1995yCat.5050....0H.
  4. ^abMason, Brian D.; et al. (2001)."The 2001 US Naval Observatory Double Star CD-ROM. I. The Washington Double Star Catalog".The Astronomical Journal.122 (6): 3466.Bibcode:2001AJ....122.3466M.doi:10.1086/323920.Vizier catalog entry
  5. ^abMallama, A. (2014). "Sloan Magnitudes for the Brightest Stars".The Journal of the American Association of Variable Star Observers.42 (2): 443.Bibcode:2014JAVSO..42..443M.Vizier catalog entry
  6. ^abGontcharov, 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.
  7. ^abTetzlaff, N.; et al. (2011)."A catalogue of young runaway Hipparcos stars within 3 kpc from the Sun".Monthly Notices of the Royal Astronomical Society.410 (1):190–200.arXiv:1007.4883.Bibcode:2011MNRAS.410..190T.doi:10.1111/j.1365-2966.2010.17434.x.S2CID 118629873.Vizier catalog entry
  8. ^Soubiran, Caroline; et al. (2016). "The PASTEL catalogue: 2016 version".Astronomy & Astrophysics.591: A118.arXiv:1605.07384.Bibcode:2016A&A...591A.118S.doi:10.1051/0004-6361/201628497.S2CID 119258214.
  9. ^abZorec, J.; et al. (2009). "Fundamental parameters of B supergiants from the BCD system".Astronomy and Astrophysics.501 (1):297–320.arXiv:0903.5134.Bibcode:2009A&A...501..297Z.doi:10.1051/0004-6361/200811147.S2CID 14969137.
  10. ^abAbt, Helmut A.; et al. (2002)."Rotational Velocities of B Stars".The Astrophysical Journal.573 (1):359–365.Bibcode:2002ApJ...573..359A.doi:10.1086/340590.
  11. ^abSeyfert, C. K.; et al. (July 1960)."A Study of the II Persei Association".Astrophysical Journal.132: 58.Bibcode:1960ApJ...132...58S.doi:10.1086/146900.
  12. ^"40 Per".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2019-07-18.
  13. ^Eggleton, 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.
  14. ^Lesh, J. R. (September 1969). "Internal motions in the associations II Per and I Lac".Astronomical Journal.74:891–898.Bibcode:1969AJ.....74..891L.doi:10.1086/110878.
  15. ^Guthrie, B. N. G. (September 1984)."The rotation of early B-type stars and the problem of star formation".Monthly Notices of the Royal Astronomical Society.210:159–171.Bibcode:1984MNRAS.210..159G.doi:10.1093/mnras/210.1.159.
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