EXOSAT observations of the X-ray pulsar 4U1145-619

Details EXOSAT observations of the X-ray pulsar 4U1145-619 EXOSAT observations of the X-ray pulsar 4U1145-619

Apr 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ssrv...40..429w&link_type=abstract

(ESA, ESLAB Symposium on X-Ray Astronomy in the EXOSAT Era, 18th, The Hague, Netherlands, Nov. 5-9, 1984) Space Science Reviews

Astronomy and Astrophysics

Astronomy

13

Exosat Satellite, Pulsars, X Ray Sources, B Stars, Binary Stars, Neutron Stars

Scientific paper

EXOSAT observations of the X-ray pulsar 4U1145-619 during June and July 1983 and July 1984 confirm that this source shows a regular 187 day outburst cycle in X rays. The results from pulse timing and X-ray spectroscopy are discussed in terms of a model for 4U1145-619 involving an eccentric binary system in which there is variable accretion from the Be primary star onto a companion neutron star.

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