Physics
Scientific paper
Nov 1977
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977natur.270..310j&link_type=abstract
Nature, vol. 270, Nov. 24, 1977, p. 310-314.
Physics
114
Conductive Heat Transfer, Neutron Stars, Stellar Mass Accretion, Stellar Models, Thermonuclear Reactions, X Ray Sources, Abundance, Binary Stars, Nuclear Fusion
Scientific paper
A description is presented of a model concerning the production of X-ray bursts by thermonuclear flashes in the freshly accreted matter near the surface of an accreting neutron star. An investigation is conducted regarding the physical processes relevant to such thermonuclear flashes. It is concluded that thermonuclear flashes may account for some, but not all, of the observed X-ray burst sources. Attention is given to a neutron star undergoing accretion of mass from a binary stellar companion, aspects of energetics, nuclear reactions, and heat transport mechanisms.
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