Short description: Star in the constellation Puppis
MX Puppis
Location of MX Puppis (circled) |
Observation data Equinox J2000.0]] (ICRS)
|
| 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[1] mas |
| Distance | 930 ± 40 ly (280 ± 10 pc) |
| Absolute magnitude (MV) | -2.97[6] |
|
| Details |
|---|
|
|---|
| Mass | 10.1[7] M☉ |
| Luminosity | 13276[8] L☉ |
| Surface gravity (log g) | 4.41[9] cgs |
| Temperature | 32,870[9] K |
| Rotational velocity (v sin i) | 145[9] km/s |
|
| Other designations |
|---|
r Puppis, CD-35°4349, GC 11197, GSC 07133-04588, HIP 40274, HR 3237, HD 68980, SAO 198957 |
| Database references |
|---|
| SIMBAD | data |
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]
A light curve for MX Puppis, adapted from Hubert and Floquet (1998)
[10]
It is a γ Cas variable, ranging from 4.92 to 4.60 magnitude.[2]
References
- ↑ 1.0 1.1 1.2 1.3 1.4 1.5 Van Leeuwen, F. (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. Vizier catalog entry
- ↑ 2.0 2.1 2.2 2.3 Samus, N. N. 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.
- ↑ 3.0 3.1 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. doi:10.1086/190820. Bibcode: 1982ApJS...50...55S.
- ↑ 4.0 4.1 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. doi:10.1134/S1063773706110065. Bibcode: 2006AstL...32..759G.
- ↑ Anderson, E.; Francis, Ch. (2012). "XHIP: An extended hipparcos compilation". Astronomy Letters 38 (5): 331. doi:10.1134/S1063773712050015. Bibcode: 2012AstL...38..331A. Vizier catalog entry
- ↑ 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. doi:10.1111/j.1365-2966.2010.17434.x. Bibcode: 2011MNRAS.410..190T. Vizier catalog entry
- ↑ Hohle, M.M.; Neuhäuser, R.; Schutz, B.F. (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. Vizier catalog entry
- ↑ 9.0 9.1 9.2 Zorec, J.; Frémat, Y.; Domiciano De Souza, A.; Royer, F.; Cidale, L.; Hubert, A.-M.; Semaan, T.; Martayan, C. et al. (2016). "Critical study of the distribution of rotational velocities of Be stars". Astronomy & Astrophysics 595: A132. doi:10.1051/0004-6361/201628760. Bibcode: 2016A&A...595A.132Z.
- ↑ 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. https://ui.adsabs.harvard.edu/abs/1998A&A...335..565H. Retrieved 25 February 2022.
 | Original source: https://en.wikipedia.org/wiki/MX Puppis. Read more |