Astronomy:CX Canis Majoris
| Observation data Equinox J2000.0]] (ICRS) | |
|---|---|
| Constellation | Canis Major |
| Right ascension | 07h 22m 00.98686s[2] |
| Declination | −25° 52′ 35.9276″[2] |
| Apparent magnitude (V) | 9.89 (-10.14) - 10.42[3] |
| Characteristics | |
| Evolutionary stage | B5V[4] |
| Variable type | Algol[3] |
| Astrometry | |
| Proper motion (μ) | RA: −2.656[2] mas/yr Dec.: 2.777[2] mas/yr |
| Parallax (π) | 0.7147 ± 0.0586[2] mas |
| Distance | 4,600 ± 400 ly (1,400 ± 100 pc) |
| Details | |
| A | |
| Mass | 5.9[5] M☉ |
| Temperature | 15,200[5] K |
| B | |
| Mass | 3.4[5] M☉ |
| Temperature | 10,600[5] K |
| Other designations | |
| Database references | |
| SIMBAD | data |
CX CMa (CX Canis Majoris) is a blue variable star in the Canis Major constellation.[6][7] Discovery of this variable is usually credited to German Astronomer Cuno Hoffmeister in 1931, although this remains uncertain.[8]
It is an eclipsing binary of Algol (detached)[3] whose magnitude varies between 9.9 and 10.4 with a period of 0.95462500 day (22.911000 hour).[7] The variability was first discovered in 1931.[9] Doubts arose because of scatter in the data and the small amplitude,[10] but the discovery was confirmed by 1949.[11] Its Algol-type light curve exhibits the O'Connell effect, meaning that there is a magnitude difference between subsequent maxima.[12]
The temperature of the secondary star has been estimated at about 10,600 K and its mass at 3.4 M☉. The spectral type of the secondary star is estimated to be in the B8 to A0 range.[13]
References
- ↑ "ASAS All Star Catalogue". The All Sky Automated Survey. http://www.astrouw.edu.pl/asas/?page=aasc.
- ↑ 2.0 2.1 2.2 2.3 2.4 Brown, A. G. A. (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics 616: A1. doi:10.1051/0004-6361/201833051. Bibcode: 2018A&A...616A...1G.
- ↑ 3.0 3.1 3.2 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: B/gcvs. Bibcode: 2009yCat....102025S.
- ↑ Williams, S. J.; Gies, D. R.; Helsel, J. W.; Matson, R. A.; Caballero-Nieves, S. (2011). "ASAS Light Curves of Intermediate-mass Eclipsing Binary Stars and the Parameters of HI Mon". The Astronomical Journal 142 (1): 5. doi:10.1088/0004-6256/142/1/5. Bibcode: 2011AJ....142....5W.
- ↑ 5.0 5.1 5.2 5.3 Nelson, Robert H.; Terrell, Dirk (2004). "CX CMa - an Early-Type Detached Eclipsing Binary". Information Bulletin on Variable Stars 5545: 1. Bibcode: 2004IBVS.5545....1N.
- ↑ 6.0 6.1 "CX CMa". SIMBAD Astronomical Database. Strasbourg Astronomical Data Center. http://simbad.u-strasbg.fr/simbad/sim-id?Ident=CX%20CMa. Retrieved 2016-09-01.
- ↑ 7.0 7.1 "VSX: Detail for CX CMa". The International Variable Star Index. American Association of Variable Star Observers. https://www.aavso.org/vsx/index.php?view=detail.top&oid=5277. Retrieved 2016-09-01.
- ↑ Milone, E. F. (1984). "Photometry &Spectroscopy of Southern O'Connell Effect Systems VY Cru, CX CMa, TU Cru, AQ Mon, &DQ Vel". Bulletin of the American Astronomical Society 16: 506. Bibcode: 1984BAAS...16..506M.
- ↑ Hoffmeister, C. (1931). "316 neue Veränderliche". Astronomische Nachrichten 242 (7): 131. doi:10.1002/asna.19312420702. Bibcode: 1931AN....242..129H.
- ↑ Florya, N. (1937). "Untersuchungen von 77 veränderlichen Sternen in Monoceros, Canis major und Puppis". Trudy Gosudarstvennogo Astronomicheskogo Instituta Im. P.K. Sternberga; T. 8 8 (2): 5. Bibcode: 1937TrSht...8....5F.
- ↑ Deurinck, R. (1949). "Fourteen New Variable Stars in Canis Major, Puppis and Monoceros". Publications du Laboratoire d'Astronomie et de Géodésie de l'Université de Louvain 12 (1ll): E17. Bibcode: 1949PLAGL..12E..17D.
- ↑ E. F. Milone (1984). "Photometry and Spectroscopy of Southern O'Connell Effect Systems VY Cru, CX CMa, TU Cru, AQ Mon, and DQ Vel". Bulletin of the American Astronomical Society 16: 506. Bibcode: 1984BAAS...16..506M.
- ↑ Robert H. Nelson, Dirk Terrell (30 July 2004). "CX CMa - an early type detached eclipsing binary". Information Bulletin on Variable Stars 5545 (5545): 1. Bibcode: 2004IBVS.5545....1N.
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