X-ray pulsars from supernova explosions

Details X-ray pulsars from supernova explosions X-ray pulsars from supernova explosions

Sep 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001esasp.459..195g&link_type=abstract

In: Exploring the gamma-ray universe. Proceedings of the Fourth INTEGRAL Workshop, 4-8 September 2000, Alicante, Spain. Editor:

Computer Science

X-Ray Pulsars, Supernovae: Explosions

Scientific paper

A comparative analysis of the samples of X-ray pulsars and galactic SNRs shows that a significant number of objects of the two samples are correlated. We show the evidence that roughly 47% of the actual sample of galactic X-ray pulsars (88) in binary systems can be the compact remnants of supernova explosions occurred in progenitor massive close binary systems, as suggested by us since 1993 with a smaller sample.

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