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MZ Puppis

From Wikipedia, the free encyclopedia
Red supergiant star in the constellation of Puppis
MZ Puppis

Alight curve for MZ Puppis, plotted fromHipparcos data[1]
Observation data
Epoch J2000.0      Equinox J2000.0
ConstellationPuppis
Right ascension08h 04m 16.19s[2]
Declination−32° 40′ 29.4″[2]
Apparent magnitude (V)5.20 - 5.44[3]
Characteristics
Evolutionary stageRed supergiant
Spectral typeM1Iab-Ib[4]
Variable typeLC?[3]
Astrometry
Radial velocity (Rv)+35.90[5] km/s
Proper motion (μ)RA: −5.736[2]mas/yr
Dec.: +6.830[2]mas/yr
Parallax (π)0.8126±0.1013 mas[2]
Distanceapprox. 4,000 ly
(approx. 1,200 pc)
Absolute magnitude (MV)−4.8[6]
Details
Mass14[7] M
Radius400[8] R
Luminosity26,550 - 28,580[8] L
Surface gravity (log g)−0.92[9] cgs
Temperature3,745±170[8] K
Age25[10] Myr
Database references
SIMBADdata

MZ Puppis is ared supergiant star in the constellation ofPuppis. It has a radius of 400 R[8] and a mass of 14solar masses, similar toBetelgeuse.

References

[edit]
  1. ^"Hipparcos Tools Interactive Data Access".Hipparcos. ESA. Retrieved8 December 2021.
  2. ^abcdeVallenari, A.; et al. (Gaia collaboration) (2023)."Gaia Data Release 3. Summary of the content and survey properties".Astronomy and Astrophysics.674: A1.arXiv:2208.00211.Bibcode:2023A&A...674A...1G.doi:10.1051/0004-6361/202243940.S2CID 244398875. Gaia DR3 record for this source atVizieR.
  3. ^abSamus, N. N.; Durlevich, O. V.; 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: B/gcvs.Bibcode:2009yCat....102025S.
  4. ^Keenan, Philip C.; McNeil, Raymond C. (1989). "The Perkins catalog of revised MK types for the cooler stars".Astrophysical Journal Supplement Series.71: 245.Bibcode:1989ApJS...71..245K.doi:10.1086/191373.
  5. ^Gontcharov, G. A. (November 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.
  6. ^Melnik, A. M.; Dambis, A. K. (2020). "Distance scale for high-luminosity stars in OB associations and in field with Gaia DR2. Spurious systematic motions".Astrophysics and Space Science.365 (7): 112.arXiv:2006.14649.Bibcode:2020Ap&SS.365..112M.doi:10.1007/s10509-020-03827-0.S2CID 220128144.
  7. ^Kervella, Pierre; Arenou, Frédéric; Thévenin, Frédéric (2022)."Stellar and substellar companions fromGaia EDR3".Astronomy & Astrophysics.657: A7.arXiv:2109.10912.Bibcode:2022A&A...657A...7K.doi:10.1051/0004-6361/202142146.eISSN 1432-0746.ISSN 0004-6361.
  8. ^abcdMessineo, M.; Brown, A. G. A. (2019)."A Catalog of Known Galactic K-M Stars of Class I Candidate Red Supergiants in Gaia DR2".The Astronomical Journal.158 (1): 20.arXiv:1905.03744.Bibcode:2019AJ....158...20M.doi:10.3847/1538-3881/ab1cbd.S2CID 148571616.
  9. ^Stassun, Keivan G.; et al. (September 2018)."The TESS Input Catalog and Candidate Target List".The Astronomical Journal.156 (3): 102.arXiv:1706.00495.Bibcode:2018AJ....156..102S.doi:10.3847/1538-3881/aad050.ISSN 0004-6256.S2CID 73582386.
  10. ^Tetzlaff, N.; Neuhäuser, R.; Hohle, M. M. (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.
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