OU Andromedae
Appearance
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Andromeda |
Right ascension | 23h 49m 40.961s[1] |
Declination | +36° 25′ 31.01″[1] |
Apparent magnitude (V) | 5.87 - 5.94[2] |
Characteristics | |
Spectral type | G1IIIe |
B−V color index | 0.79 |
Variable type | FK Com[2] |
Astrometry | |
Radial velocity (Rv) | 0.7 km/s |
Proper motion (μ) | RA: 1.01 ± 0.41[1] mas/yr Dec.: -47.59 ± 0.26[1] mas/yr |
Parallax (π) | 7.71 ± 0.34 mas[1] |
Distance | 420 ± 20 ly (130 ± 6 pc) |
Details | |
Mass | 2.9[3] M☉ |
Other designations | |
Database references | |
SIMBAD | data |
OU Andromedae is a rotationally variable star. It has an X-ray emission of 8.2 × 1030 erg s−1.[3] Varying between magnitudes 5.87 and 5.94, it has been classified as an FK Comae Berenices variable.
References
- ^ a b c d e van Leeuwen, F. (2007). "Validation of the new Hipparcos reduction". Astronomy and Astrophysics. 474 (2): 653–664. arXiv:0708.1752. Bibcode:2007A&A...474..653V. doi:10.1051/0004-6361:20078357.Vizier catalog entry
- ^ a b 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. Bibcode:2009yCat....102025S.
- ^ a b Gondoin, P. (December 1999), "Evolution of X-ray activity and rotation on G-K giants", Astronomy and Astrophysics, 352: 217–227, Bibcode:1999A&A...352..217G