Observation data Epoch J2000.0 Equinox J2000.0 |
|
---|---|
Constellation | Perseus |
Right ascension | 03h 55m 23.07715s |
Declination | +31° 02′ 450062″ |
Apparent magnitude (V) | 6.778(6.03 - 7.00) |
Characteristics | |
Spectral type | O9.5IIIe-B0Ve |
U−B color index | −0.790 |
B−V color index | +0.137 |
Variable type | γ Cas + X-ray pulsar |
Astrometry | |
Radial velocity (Rv) | −50.00 km/s |
Proper motion (μ) |
RA: −2.28 mas/yr Dec.: −5.42 mas/yr |
Parallax (π) | 2.34 ± 0.70mas |
Distance | 950pc |
Absolute magnitude (MV) | −3.47 |
Orbit | |
Primary | X Per |
Companion | 4U 0352+309 |
Period (P) | 250.3 days |
Semi-major axis (a) | 2.2 AU |
Eccentricity (e) | 0.111 |
Inclination (i) | 23 - 30° |
Details | |
Mass | 15.5 M☉ |
Radius | 6.5 R☉ |
Luminosity | 29,000 L☉ |
Surface gravity (log g) | 4.0 cgs |
Temperature | 29,500 K |
Rotational velocity (v sin i) | 215 km/s |
Age | 5 Myr |
Other designations | |
A: X Per | |
B: 4U 0352+309 | |
Database references | |
SIMBAD | data |
X Persei is a binary star system located in the constellation Perseus, approximately 950 parsecs away.
The optical star X Persei has been classified either as an O-type giant or a B-type main sequence star. It is a Be star, rotating rapidly, and at times surrounded by a disk of expelled material. This qualifies it as a Gamma Cassiopeia variable, and the visual range is magnitude 6 - 7. There is a faint optical companion separated by 22.5" which the Catalog of Components of Double and Multiple Stars refers to as X Persei B.
X Persei A is in orbit with a neutron star, which is catalogued as 4U 0352+309 in the final Uhuru catalog of X-ray objects. It is a pulsar with an unusually long period of 837 seconds.