Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Andromeda |
Right ascension | 00h 30m 05.8084s[2] |
Declination | +26° 17′ 26.4389″[2] |
Apparent magnitude (V) | 14.04 – 17.00 variable[3] |
Characteristics | |
Spectral type | pec(UG)[3] |
Apparent magnitude (B) | 11.84[4] |
Apparent magnitude (R) | 14.69[4] |
Apparent magnitude (G) | 14.8494[2] |
Apparent magnitude (J) | 14.652[5] |
Apparent magnitude (H) | 14.485[5] |
Apparent magnitude (K) | 14.344[5] |
Variable type | SW Sex[4] |
Astrometry | |
Proper motion (μ) | RA: −10.924±0.081 [2] mas/yr Dec.: −10.992±0.052[2] mas/yr |
Parallax (π) | 1.2323 ± 0.0437 mas[2] |
Distance | 2,650 ± 90 ly (810 ± 30 pc) |
Orbit | |
Period (P) | 3.5112 hours[6] |
Other designations | |
Database references | |
SIMBAD | data |
PX Andromedae (often abbreviated to PX And) is an eclipsing cataclysmic variable star in the constellation Andromeda. It has been classified as a SW Sextantis variable,[4] and its apparent visual magnitude varies between 14.04 and 17.[3]
In 1982, Richard Green et al. listed PX Andromedae as a possible cataclysmic variable, based on spectra taken with the Hale Telescope.[7] Observations in 1989 by Li Yong et al, at the Beijing Observatory detected rapid variations of the star's brightness of up to 0.2 magnitudes, as well as eclipses which occur every 3.5 hours.[8] In 1992 the star was given the variable star designation PX Andromedae.[9]
stanishev
was invoked but never defined (see the help page).GCVS
was invoked but never defined (see the help page).SuperWASP
was invoked but never defined (see the help page).2MASS Cat
was invoked but never defined (see the help page).Thomas2010
was invoked but never defined (see the help page).Green1982
was invoked but never defined (see the help page).Li1990
was invoked but never defined (see the help page).Kazarovets1993
was invoked but never defined (see the help page).