(Redirected from O Persei )
Star in the constellation Perseus
This article is about o Persei. Not to be confused with ο (omicron) Persei .
40 Persei
Location of 40 Persei (circled)
Observation dataEpoch J2000 Equinox J2000
Constellation
Perseus
Right ascension
03 42 22.64555
Declination
33° 57′ 54.0893″
Apparent magnitude (V)
4.97
Characteristics
Spectral type
B0.5V + A1Vn
U−B color index
−0.84
B−V color index
+0.00
Astrometry Radial velocity (Rv )+22.00 km/s Proper motion (μ) RA: +2.71 mas /yr Dec.: −5.91 mas /yr Parallax (π)3.09 ± 0.21 mas Distance 1,060 ± 70 ly (320 ± 20 pc ) Absolute magnitude (MV )−2.26
Details 40 Per A Mass 12.5 M ☉ Luminosity 936 L ☉ Surface gravity (log g )4.36 cgs Temperature 29,330 K Metallicity −0.43 dex Rotational velocity (v sin i )10 km/s Age 7.2 Myr
Other designations 40 Per , BD +33°698, GC 4420, HD 22951, HIP 17313, HR 1123, SAO 56646, CCDM J03424+3358A, WDS J03424+3358A
Database references SIMBAD data
40 Persei is a wide binary star system in the northern constellation of Perseus . It has the Bayer designation ο Persei , while 40 Persei is the Flamsteed designation . The system is visible to the naked eye as a faint, blue-white hued point of light with an apparent visual magnitude of 4.97. It is located approximately 1060 light years away from the Sun based on parallax , and is drifting further away with a radial velocity of +22 km/s. The system is a member of the Perseus OB2 association of co-moving stars.
The primary component is a massive B-type main-sequence star with a stellar classification of B0.5V. It is about 7.2 million years old and has a very low projected rotational velocity for an early B-type star, measured at 10 km/s. This star has 12.5 times the mass of the Sun and is radiating 936 times the Sun's luminosity from its photosphere at an effective temperature of 29,330 K. The companion is magnitude 10.04, A-type main-sequence star with a class of A1Vn, and is located at an angular separation of 19.8″ from the primary.
References
^ Van 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
^ 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 . Vizier catalog entry
^ Hoffleit, 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 .
^ Mason, 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
^ Mallama, 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
^ 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 .
^ Tetzlaff, 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
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 .
^ Zorec, 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 .
^ Abt, 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 .
^ Seyfert, 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 .
"40 Per" . SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 2019-07-18.
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 .
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 .
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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