PSR B1259−63/LS 2883

PSR J1302−6350 is a pulsar and member of an eclipsing binary star system with the blue O9.5Ve-class star LS 2883. The pair has an eccentric orbit that is inclined to the line of sight from Earth by about 36°, leading to a 40-day-long eclipse each time the pulsar passes behind the star. The pulsar has a period of about 48 ms and a luminosity of 8.3 × 1035 erg/s. It emits very high energy gamma rays that vary on a time scale of several days.

LS 2883
Observation data
Epoch J2000      Equinox J2000
Constellation Centaurus
Right ascension 13h 02m 47.655s
Declination −63° 50 08.67
Apparent magnitude (V) 10.34
Characteristics
Spectral type O9.5Ve + pulsar
Astrometry
Proper motion (μ) RA: −6.0 mas/yr
Dec.: −5.7 mas/yr
Distance7,500 ly
Orbit
CompanionSS 2883
Period (P)1237 days
Eccentricity (e)0.87
Inclination (i)36°
Other designations
AAVSO 1256−63, ALS 2883, AX J1302−638, CPD-63° 2495, GSC 08997-01597, Hbg 757, Hen 3-852, INTREF 538, LS 2883, MSX6C G304.1845-00.9916, PSR B1259−63 PSR J1302−6350, THA 17-8, TYC 8997-1597-1, UCAC2 3710789, WRAY 15-1053.
Database references
SIMBADdata

The star LS 2883 has about 10 solar masses and is 6 solar radii in size. The rate of rotation is about 280 km/s at the equator, or 70% of the breakup velocity.

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