S Apodis
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Apus |
| Right ascension | 15h 09m 24.53447s[1] |
| Declination | −72° 03′ 45.1898″[1] |
| Apparent magnitude (V) | 9.7[2] |
| Characteristics | |
| Spectral type | C |
| Variable type | R Coronae Borealis variable |
| Astrometry | |
| Radial velocity (Rv) | -75.00 km/s |
| Proper motion (μ) | RA: -7.52 ± 1.28[1] mas/yr Dec.: -2.96 ± 1.53[1] mas/yr |
| Details | |
| Luminosity | 960[3] L☉ |
| Temperature | 3916[3] K |
| Other designations | |
| Database references | |
| SIMBAD | data |
S Apodis (HD 133444) is an R Coronae Borealis variable star located in the far southern constellation Apus. These are extremely hydrogen-deficient supergiants thought to have arisen as the result of the merger of two white dwarfs; fewer than 100 have been discovered as of 2012.[2] Located around 5000 light-years distant, it shines with a luminosity approximately 960 times that of the Sun and has a surface temperature of 3916 K.[3]
References
- 1 2 3 4 van Leeuwen, F. (2007). "Validation of the new Hipparcos reduction". Astronomy and Astrophysics. 474 (2): 653–64. Bibcode:2007A&A...474..653V. arXiv:0708.1752
. doi:10.1051/0004-6361:20078357.Vizier catalog entry - 1 2 Tisserand; Clayton; Welch; Pilecki; Wyrzykowski; Kilkenny (2012). "The Ongoing Pursuit of R Coronae Borealis Stars: ASAS-3 Survey Strikes Again". Astronomy & Astrophysics. 551: 22. Bibcode:2013A&A...551A..77T. arXiv:1211.2475 . doi:10.1051/0004-6361/201220713. A77.
- 1 2 3 McDonald, I.; Zijlstra, A. A.; Boyer, M. L. (2012). "Fundamental Parameters and Infrared Excesses of Hipparcos Stars". Monthly Notices of the Royal Astronomical Society. 427 (1): 343–57. Bibcode:2012MNRAS.427..343M. arXiv:1208.2037 . doi:10.1111/j.1365-2966.2012.21873.x.
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