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34 Persei

From Wikipedia, the free encyclopedia
Binary star system in the constellation Perseus
34 Persei
Location of 34 Persei (circled)
Observation data
Epoch J2000      Equinox J2000
ConstellationPerseus
Right ascension03h 29m 22.05019s[1]
Declination+49° 30′ 32.2114″[1]
Apparent magnitude (V)4.67[2](4.76 + 7.18)[3]
Characteristics
Evolutionary stageMain sequence
Spectral typeB3V[4]
U−Bcolor index−0.57[5]
B−Vcolor index−0.09[5]
Astrometry
Radial velocity (Rv)−3.50[6] km/s
Proper motion (μ)RA: +22.20[1]mas/yr
Dec.: −29.49[1]mas/yr
Parallax (π)6.05±0.36 mas[1]
Distance540 ± 30 ly
(165 ± 10 pc)
Absolute magnitude (MV)−1.62[2]
Details
32 Per A
Mass6.9±0.1[7] M
Radius3.1[8] R
Luminosity671[2] L
Surface gravity (log g)4.076[9] cgs
Temperature16,421[9] K
Rotational velocity (v sin i)200[9] km/s
Age29.3±3.4[7] Myr
Other designations
34 Per,BD+49°945,FK5 1549,GC 4133,HD 21428,HIP 16244,HR 1044,SAO 38872,CCDM J03294+4931AB,WDS J03294+4931AB[10]
Database references
SIMBADdata

34 Persei is abinary star[3] system in the northernconstellation ofPerseus. It is visible to the naked eye as a faint, blue-white hued point of light with a combinedapparent visual magnitude of 4.67.[2] The system is located approximately 540 light years away from the Sun based onparallax,[1] but it is drifting closer with aradial velocity of −3.5 km/s.[6] It is a likely member of theAlpha Persei Cluster.[11]

The primary member, designated component A, is aB-type main-sequence star with astellar classification of B3V[4] and visual magnitude 4.76.[3] It is an estimated 29[7] million years old with a high rate of spin, showing aprojected rotational velocity of 200 km/s.[9] The star has 6.9[7] times themass of the Sun and about 3.1[8] times theSun's radius. It is radiating 671[2] times theSun's luminosity from itsphotosphere at aneffective temperature of 16,421 K.[9]

The secondary companion, component B, has anangular separation of0.6 from the primary and visual magnitude of 7.34.[12]

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. ^abcdeAnderson, 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. ^abcEggleton, 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.
  4. ^abHoffleit, D.; Warren, W. H. (1995). "Bright Star Catalogue".VizieR On-line Data Catalog: V/50. Originally Published in: 1964BS....C......0H.5050 (5th Revised ed.).Bibcode:1995yCat.5050....0H.
  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. ^abcdTetzlaff, N.; et al. (January 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.
  8. ^abPasinetti Fracassini, L. E.; et al. (February 2001), "Catalogue of Apparent Diameters and Absolute Radii of Stars (CADARS)",Astronomy and Astrophysics,367 (2) (Third ed.):521–524,arXiv:astro-ph/0012289,Bibcode:2001A&A...367..521P,doi:10.1051/0004-6361:20000451,S2CID 425754
  9. ^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.
  10. ^"34 Per".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2019-07-12.
  11. ^Zuckerman, B.; et al. (June 2012). "Stellar Membership and Dusty Debris Disks in the α Persei Cluster".The Astrophysical Journal.752 (1): 12.arXiv:1204.3950.Bibcode:2012ApJ...752...58Z.doi:10.1088/0004-637X/752/1/58.S2CID 119207634. 58.
  12. ^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
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