| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| 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 mas [2] |
| 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 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. Retrieved 8 December 2021.
- ^ a b c d e Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv: 1804.09365. Bibcode: 2018A&A...616A...1G. doi: 10.1051/0004-6361/201833051.
- ^ 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: 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. arXiv: 1104.3166. Bibcode: 2011AJ....142....5W. doi: 10.1088/0004-6256/142/1/5. S2CID 119229809.
- ^ a b c d 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.
- ^ a b "CX CMa". SIMBAD Astronomical Database. Strasbourg Astronomical Data Center. Retrieved 2016-09-01.
- ^ a b "VSX: Detail for CX CMa". The International Variable Star Index. American Association of Variable Star Observers. 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. Bibcode: 1931AN....242..129H. doi: 10.1002/asna.19312420702.
- ^ 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.
| Stars |
| ||||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| |||||||||||||
|
Star clusters |
| ||||||||||||
| |||||||||||||
| Galaxies |
| ||||||||||||
| |||||||||||||
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| 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 mas [2] |
| 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 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. Retrieved 8 December 2021.
- ^ a b c d e Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv: 1804.09365. Bibcode: 2018A&A...616A...1G. doi: 10.1051/0004-6361/201833051.
- ^ 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: 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. arXiv: 1104.3166. Bibcode: 2011AJ....142....5W. doi: 10.1088/0004-6256/142/1/5. S2CID 119229809.
- ^ a b c d 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.
- ^ a b "CX CMa". SIMBAD Astronomical Database. Strasbourg Astronomical Data Center. Retrieved 2016-09-01.
- ^ a b "VSX: Detail for CX CMa". The International Variable Star Index. American Association of Variable Star Observers. 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. Bibcode: 1931AN....242..129H. doi: 10.1002/asna.19312420702.
- ^ 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.
| Stars |
| ||||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| |||||||||||||
|
Star clusters |
| ||||||||||||
| |||||||||||||
| Galaxies |
| ||||||||||||
| |||||||||||||