Star in the constellation Puppis
MX Puppis (MX Pup ) is a class B1.5IV[ 3] (blue subgiant) star in the constellation Puppis . Its apparent magnitude varies irregularly between magnitude 4.6 and 4.9 and it is classified as a Gamma Cassiopeiae variable .[ 2] It is approximately 930 light years away based on parallax.[ 1]
MX Puppis was first found to be a variable star by Alan William James Cousins in 1959.[ 11] It was given its variable star designation in 1972.[ 12]
A light curve for MX Puppis, adapted from Hubert and Floquet (1998)[ 13]
^ a b c d e f Van 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
^ a b c Samus, 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 . Bibcode :2009yCat....102025S .
^ a b Slettebak, A. (1982). "Spectral types and rotational velocities of the brighter Be stars and A-F type shell stars" . Astrophysical Journal Supplement Series . 50 : 55. Bibcode :1982ApJS...50...55S . doi :10.1086/190820 .
^ a b 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 .
^ Gontcharov, 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 .
^ Anderson, 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
^ a b Tetzlaff, N.; Neuhäuser, R.; Hohle, M. M. (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 . Vizier catalog entry
^ Vallenari, 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 at VizieR .
^ Balona, L. A.; Ozuyar, D. (2020). "Pulsation among TESS a and B stars and the Maia variables" . Monthly Notices of the Royal Astronomical Society . 493 (4): 5871. arXiv :2001.04497 . Bibcode :2020MNRAS.493.5871B . doi :10.1093/mnras/staa670 . S2CID 210472317 .
^ a b c Zorec, J.; Frémat, Y.; Domiciano De Souza, A.; Royer, F.; Cidale, L.; Hubert, A.-M.; Semaan, T.; Martayan, C.; Cochetti, Y. R.; Arias, M. L.; Aidelman, Y.; Stee, P. (2016). "Critical study of the distribution of rotational velocities of Be stars" . Astronomy & Astrophysics . 595 : A132. Bibcode :2016A&A...595A.132Z . doi :10.1051/0004-6361/201628760 . hdl :11336/37946 .
^ Cite error: The named reference Cousins
was invoked but never defined (see the help page ).
^ Cite error: The named reference Kukarkin
was invoked but never defined (see the help page ).
^ Cite error: The named reference Hubert1998
was invoked but never defined (see the help page ).