Astronomy:10 Persei
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Short description: Blue-supergiant star in the constellation Perseus
  | |
| Observation data Equinox J2000.0]] (ICRS) | |
|---|---|
| Constellation | Perseus |
| Right ascension | 02h 25m 16.02916s[1] |
| Declination | +56° 36′ 35.3536″[1] |
| Apparent magnitude (V) | 6.26[2] |
| Characteristics | |
| Evolutionary stage | Blue supergiant |
| Spectral type | B2Ia[3] |
| U−B color index | −0.61[2] |
| B−V color index | +0.30[2] |
| Variable type | α Cyg[4] |
| Astrometry | |
| Radial velocity (Rv) | −46.0[5] km/s |
| Proper motion (μ) | RA: −0.08[1] mas/yr Dec.: −1.50[1] mas/yr |
| Parallax (π) | 0.30 ± 0.41[6] mas |
| Absolute magnitude (MV) | −6.70[7] |
| Details[7] | |
| Mass | 26 M☉ |
| Radius | 51.4 R☉ |
| Luminosity | 250,000 L☉ |
| Surface gravity (log g) | 2.38 cgs |
| Temperature | 18,000 K |
| Rotational velocity (v sin i) | 82 km/s |
| Other designations | |
| Database references | |
| SIMBAD | data |
10 Persei is a blue supergiant star in the constellation Perseus. Its apparent magnitude is 6.26 although it is slightly variable.
10 Persei is located around 3,333 parsecs (10,870 ly) distant in the Perseus OB1 stellar association. It lies close to the Double Cluster and is considered a cluster member.[8]
In 1999, 10 Persei was given the variable star designation V554 Persei, after being identified as varying in Hipparcos photometry.[10] Its brightness varies by less than a tenth of a magnitude with no clear period.[4]
References
- ↑ 1.0 1.1 1.2 1.3 Van Leeuwen, F. (2007). "Validation of the new Hipparcos reduction". Astronomy and Astrophysics 474 (2): 653–664. doi:10.1051/0004-6361:20078357. Bibcode: 2007A&A...474..653V.
- ↑ 2.0 2.1 2.2 Ducati, J. R. (2002). "VizieR Online Data Catalog: Catalogue of Stellar Photometry in Johnson's 11-color system". CDS/ADC Collection of Electronic Catalogues 2237. Bibcode: 2002yCat.2237....0D.
- ↑ Kraus, M.; Borges Fernandes, M.; Kubát, J. (2009). "Parameters of galactic early B supergiants. The influence of the wind on the interstellar extinction determination". Astronomy and Astrophysics 499 (1): 291. doi:10.1051/0004-6361/200810319. Bibcode: 2009A&A...499..291K.
- ↑ 4.0 4.1 Samus, N. N. et al. (2009). "VizieR Online Data Catalog: General Catalogue of Variable Stars (Samus+ 2007-2013)". VizieR On-line Data Catalog: B/GCVS. Originally Published in: 2009yCat....102025S 1. Bibcode: 2009yCat....102025S.
- ↑ Wilson, Ralph Elmer (1953). "General catalogue of stellar radial velocities". Washington. Bibcode: 1953GCRV..C......0W.
- ↑ Gaia Collaboration (2016). "VizieR Online Data Catalog: Gaia DR1 (Gaia Collaboration, 2016)". VizieR On-line Data Catalog: I/337. Originally Published in: Astron. Astrophys. 1337. Bibcode: 2016yCat.1337....0G.
- ↑ 7.0 7.1 Searle, S. C.; Prinja, R. K.; Massa, D.; Ryans, R. (2008). "Quantitative studies of the optical and UV spectra of Galactic early B supergiants. I. Fundamental parameters". Astronomy and Astrophysics 481 (3): 777. doi:10.1051/0004-6361:20077125. Bibcode: 2008A&A...481..777S.
- ↑ Lee, Hsu-Tai; Lim, Jeremy (2008). "On the Formation of Perseus OB1 at High Galactic Latitudes". The Astrophysical Journal 679 (2): 1352–1363. doi:10.1086/587801. Bibcode: 2008ApJ...679.1352L.
- ↑ "Hipparcos Tools Interactive Data Access". ESA. https://www.cosmos.esa.int/web/hipparcos/interactive-data-access.
- ↑ Kazarovets, E. V.; Samus, N. N.; Durlevich, O. V.; Frolov, M. S.; Antipin, S. V.; Kireeva, N. N.; Pastukhova, E. N. (1999). "The 74th Special Name-list of Variable Stars". Information Bulletin on Variable Stars 4659: 1. Bibcode: 1999IBVS.4659....1K.
Further reading
- Crowther, P. A.; Lennon, D. J.; Walborn, N. R. (2006). "Physical parameters and wind properties of galactic early B supergiants". Astronomy and Astrophysics 446 (1): 279–293. doi:10.1051/0004-6361:20053685. Bibcode: 2006A&A...446..279C.
- McErlean, N. D.; Lennon, D. J.; Dufton, P. L. (1999). "Galactic B-supergiants: A non-LTE model atmosphere analysis to estimate atmospheric parameters and chemical compositions". Astronomy and Astrophysics 349: 553. Bibcode: 1999A&A...349..553M.
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