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Nature of the compact X-ray source in supernova remnant RCW103 and related problems

S. B. Popov
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Abstract

I discuss the nature of the compact X-ray source in the center of the supernova remnant RCW 103. Several models, based on the accretion onto a compact object are analyzed. I show that it is more likely that the central X-ray source is an accreting neutron star than an accreting black hole. I also argue that models of a disrupted binary system consisting of an old accreting neutron star and a new one observed as a 69-ms pulsar are most favored.

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S. B. Popov. 1999-12-30. Nature of the compact X-ray source in supernova remnant RCW103 and related problems. https://doi.org/10.1023/a%3A1026528829858

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