Thermonuclear flashes in the accreting envelope of a hot neutron star. I. Accretion rate M = 1017 g/sec

Details Thermonuclear flashes in the accreting envelope of a hot neutron star. I. Accretion rate M = 1017 g/sec Thermonuclear flashes in the accreting envelope of a hot neutron star. I. Accretion rate M = 1017 g/sec

Oct 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983azh....60..909k&link_type=abstract

Astronomicheskii Zhurnal, Vol. 60, p.909

Astronomy and Astrophysics

Astronomy

2

Scientific paper

The results of calculations concerning the accretion of matter and the following thermonuclear flash on the surface of a hot neutron star are presented. The influence of the neutron star luminosity and of the initial chemical composition of the accreted matter on the properties of the flash are investigated. It is shown that under the same initial thermal conditions, the evolution of the flash depends mainly on the helium abundance in the accreted layer prior to the development of thermal instability.

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