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MX 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
Location of MX Puppis (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Puppis
Right ascension 08h 13m 29.51720s[1]
Declination −35° 53′ 58.2662″[1]
Apparent magnitude (V) 4.60 - 4.92[2]
Characteristics
Spectral type B1.5 IVe[3]
U−B color index −0.98[4]
B−V color index −0.11[4]
Variable type γ Cas[2]
Astrometry
Radial velocity (Rv)+35.00[5] km/s
Proper motion (μ) RA: −7.30[1] mas/yr
Dec.: +9.75[1] mas/yr
Parallax (π)3.51 ± 0.16 mas[1]
Distance930 ± 40 ly
(280 ± 10 pc)
Absolute magnitude (MV)−2.97[6]
Details
Mass10.1[7] M
Radius6.5[8] R
Luminosity28,840[9] L
Surface gravity (log g)4.41[10] cgs
Temperature32,870[10] K
Rotational velocity (v sin i)145[10] km/s
Age22.5[7] Myr
Other designations
r Puppis, CD−35°4349, GC 11197, GSC 07133-04588, HIP 40274, HR 3237, HD 68980, SAO 198957
Database references
SIMBADdata
A light curve for MX Puppis, adapted from Hubert and Floquet (1998)[11]

MX Puppis is a γ Cas variable, ranging from 4.92 to 4.60 magnitude.[2]

References edit

  1. ^ 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
  2. ^ a b c d 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.
  3. ^ 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.
  4. ^ 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.
  5. ^ 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.
  6. ^ 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
  7. ^ 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
  8. ^ 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.
  9. ^ 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.
  10. ^ 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.
  11. ^ Hubert, A. M.; Floquet, M. (July 1998). "Investigation of the variability of bright Be stars using Hipparcos photometry". Astronomy and Astrophysics. 335: 565–572. Bibcode:1998A&A...335..565H. Retrieved 25 February 2022.


puppis, confused, with, puppis, puppis, class, blue, subgiant, star, constellation, puppis, apparent, magnitude, varies, irregularly, between, magnitude, classified, gamma, cassiopeiae, variable, approximately, light, years, away, based, parallax, location, ci. Not to be confused with R Puppis or Rho 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 PuppisLocation of MX Puppis circled Observation dataEpoch J2000 Equinox J2000 Constellation Puppis Right ascension 08h 13m 29 51720s 1 Declination 35 53 58 2662 1 Apparent magnitude V 4 60 4 92 2 Characteristics Spectral type B1 5 IVe 3 U B color index 0 98 4 B V color index 0 11 4 Variable type g Cas 2 AstrometryRadial velocity Rv 35 00 5 km sProper motion m RA 7 30 1 mas yr Dec 9 75 1 mas yrParallax p 3 51 0 16 mas 1 Distance930 40 ly 280 10 pc Absolute magnitude MV 2 97 6 DetailsMass10 1 7 M Radius6 5 8 R Luminosity28 840 9 L Surface gravity log g 4 41 10 cgsTemperature32 870 10 KRotational velocity v sin i 145 10 km sAge22 5 7 Myr Other designationsr Puppis CD 35 4349 GC 11197 GSC 07133 04588 HIP 40274 HR 3237 HD 68980 SAO 198957 Database referencesSIMBADdata A light curve for MX Puppis adapted from Hubert and Floquet 1998 11 MX Puppis is a g Cas variable ranging from 4 92 to 4 60 magnitude 2 References edit 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 amp A 474 653V doi 10 1051 0004 6361 20078357 S2CID 18759600 Vizier catalog entry a b c d 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 Neuhauser 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 amp 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 Fremat 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 amp Astrophysics 595 A132 Bibcode 2016A amp A 595A 132Z doi 10 1051 0004 6361 201628760 hdl 11336 37946 Hubert A M Floquet M July 1998 Investigation of the variability of bright Be stars using Hipparcos photometry Astronomy and Astrophysics 335 565 572 Bibcode 1998A amp A 335 565H Retrieved 25 February 2022 nbsp This subgiant star related article is a stub You can help Wikipedia by expanding it vte nbsp This variable star related article is a stub You can help Wikipedia by expanding it vte Retrieved from https en wikipedia org w index php title MX Puppis amp oldid 1195781715, wikipedia, wiki, book, books, library,

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