PT Puppis

PT Puppis (PT Pup) is a star in the constellation Puppis. Anamarija Stankov confirmed this star as a Beta Cephei variable.[4] 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.[3]

PT Puppis

A light curve for PT Puppis, plotted from TESS data[1]
Observation data
Epoch J2000      Equinox J2000
Constellation Puppis
Right ascension 07h 36m 41.03388s[2]
Declination 19° 42 08.4211[2]
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 mas[2]
Distanceapprox. 1,700 ly
(approx. 520 pc)
Details
Mass7.94[3] M
Luminosity6405[3] L
Temperature19400[3] K
Other designations
PT Puppis, HR 2928, HD 61068, HIP 37036, SAO 153149
Database references
SIMBADdata

References

  1. "MAST: Barbara A. Mikulski Archive for Space Telescopes". Space Telescope Science Institute. Retrieved 8 December 2021.
  2. van Leeuwen, F. (November 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
  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, arXiv:1003.2335, Bibcode:2010AN....331..349H, doi:10.1002/asna.200911355, S2CID 111387483
  4. Stankov, Anamarija; Handler, Gerald (2005). "Catalog of Galactic β Cephei Stars". The Astrophysical Journal Supplement Series. 158 (2): 193–216. arXiv:astro-ph/0506495. Bibcode:2005ApJS..158..193S. doi:10.1086/429408. ISSN 0067-0049. S2CID 119526948.


This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.