Astronomy:PT Puppis
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Short description: Star in the constellation Puppis
| Observation data Equinox J2000.0]] (ICRS) | |
|---|---|
| Constellation | Puppis |
| Right ascension | 07h 36m 41.03388s[2] |
| Declination | −19° 42′ 08.4211″[2] |
| Apparent magnitude (V) | 5.720–5.740[3] |
| Characteristics | |
| Spectral type | B2 II |
| Variable type | Beta Cephei |
| Astrometry | |
| Radial velocity (Rv) | +22.00 ± 4.3 km/s |
| Proper motion (μ) | RA: −7.86 ± 0.21[2] mas/yr Dec.: 5.81 ± 0.20[2] mas/yr |
| Parallax (π) | 1.93 ± 0.28[2] mas |
| Distance | approx. 1,700 ly (approx. 520 pc) |
| Details | |
| Mass | 7.94[4] M☉ |
| Luminosity | 6405[4] L☉ |
| Temperature | 19400[4] K |
| Other designations | |
PT Puppis, HR 2928, HD 61068, HIP 37036, SAO 153149 | |
| Database references | |
| SIMBAD | data |
PT Puppis (PT Pup) is a star in the constellation Puppis. Anamarija Stankov confirmed this star as a Beta Cephei variable.[5] Analysis of its spectrum and allowing for extinction gives a mass 7.94 times that of the Sun, a surface temperature of 19,400 K and luminosity of 6405 Suns.[4]
References
- ↑ "MAST: Barbara A. Mikulski Archive for Space Telescopes". Space Telescope Science Institute. https://mast.stsci.edu/portal/Mashup/Clients/Mast/Portal.html.
- ↑ 2.0 2.1 2.2 2.3 2.4 van Leeuwen, F. (November 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
- ↑ "GCVS catalog (GCVS 5.1, version Oct, 2020)". https://vizier.cds.unistra.fr/viz-bin/VizieR-S?V*%20PT%20Pup.
- ↑ 4.0 4.1 4.2 4.3 Hohle, M. M.; Neuhäuser, R.; Schutz, B. F. (April 2010), "Masses and luminosities of O- and B-type stars and red supergiants", Astronomische Nachrichten 331 (4): 349, doi:10.1002/asna.200911355, Bibcode: 2010AN....331..349H
- ↑ Stankov, Anamarija; Handler, Gerald (2005). "Catalog of Galactic β Cephei Stars". The Astrophysical Journal Supplement Series 158 (2): 193–216. doi:10.1086/429408. ISSN 0067-0049. Bibcode: 2005ApJS..158..193S.
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