The binary X-ray pulsar 3U 1538-52

Details The binary X-ray pulsar 3U 1538-52 The binary X-ray pulsar 3U 1538-52

Dec 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977mnras.181p..73d&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 181, Dec. 1977, p. 73P-79P. Research supported by the Science Research

Astronomy and Astrophysics

Astronomy

23

Binary Stars, Companion Stars, Pulsars, X Ray Sources, Ariel Satellites, Latitude Measurement, Light Curve, Oso, Radial Velocity, Stellar Winds, Supergiant Stars, X Ray Spectroscopy

Scientific paper

Ariel 5 SSI and Experiment C observations of 3U 1538-52 are presented which confirm the binary nature of this source and resolve its positional uncertainty. Combining Ariel 5 data with that from OSO-8 leads to improve estimates of the orbital parameters which are discussed in terms of the implications for the mass and radius of the as yet unidentified companion star.

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