X-ray binaries and the asymmetry of supernova outbursts

Details X-ray binaries and the asymmetry of supernova outbursts X-ray binaries and the asymmetry of supernova outbursts

Jun 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975sval....1...99a&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 1, May 1975, p. 19-23.) Soviet Astronomy Letters, vol. 1, May-June 1975, p. 99, 100. Tr

Astronomy and Astrophysics

Astronomy

Binary Stars, Stellar Evolution, Supernova Remnants, X Ray Binaries, X Ray Stars, Giant Stars, Gravitational Collapse, Milky Way Galaxy, X Ray Sources

Scientific paper

It is noted that only about one-thousandth of all close binary systems survive after the collapse of one component. On this basis, it is estimated that about 100 strong and 1000 weak X-ray sources probably exist in our galaxy. The evolution of close binary systems is reviewed together with the formation of collapsars. It is shown that binary systems are destroyed due to the asymmetry of supernova explosions. In the case of such an explosion, the collapsed star is estimated to receive 0.05 to 0.15 of the total momentum of the exploding envelope.

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