V803 Centauri (V803 Cen) is a cataclysmic binary consisting of a dwarf helium star losing mass to a white dwarf. It is an example of the AM Canum Venaticorum (AM CVn) type of cataclysmic variable stars.[1]
Three light curves for V803 Centauri, on three timescales, hours (plot A), days (plot B) and years (plot C). Adapted from Patterson et al. (2000),[1] Kato et al. (2004)[2] and Levitan et al. (2015)[3] | |
| Observation data Epoch J2000.0 Equinox J2000.0 | |
|---|---|
| Constellation | Centaurus |
| Right ascension | 13h 23m 44.54s[4] |
| Declination | −41° 44′ 29.5″[5] |
| Apparent magnitude (V) | 13.2[6] (var) |
| Characteristics | |
| Spectral type | pec |
| U−B color index | -0.9 - -1.0[7] |
| B−V color index | 0.0.1[7] |
| Variable type | AM CVn[8] |
| Astrometry | |
| Distance | 347[8] pc |
| Absolute magnitude (MV) | 5.93[8] |
| Details | |
| Mass | 0.9-1.2/0.06-0.11[8] M☉ |
| Other designations | |
| Database references | |
| SIMBAD | data |
Constellation of Centaurus | |||||
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