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[en] The author reviews the progress achieved in developing the thermonuclear flash model of X-ray burst sources. Numerical calculations have been remarkably successful in accounting for the general properties of the bursts from most X-ray burst sources. Moreover, the theoretical work to date suggests that the characteristics of X-ray bursts should be capable of imparting substantial constraints on the properties of the underlying neutronstatrs. (Auth.)
Source
Sugimoto, D. (Tokyo Univ. (Japan)); Lamb, D.Q. (Harvard Univ., Cambridge, MA (USA). Center for Astrophysics); Schramm, D.N. (Chicago Univ., IL (USA)) (eds.); International Astronomical Union; 362 p; ISBN 90-277-1274-3; 
; 1981; p. 207-227; D. Reidel; Dordrdrecht, Netherlands; International Astronomical Union symposium no. 93 on fundamental problems in the theory of stellar evolution; Kyoto, Japan; 22 - 25 Jul 1980; 50 refs.
; 1981; p. 207-227; D. Reidel; Dordrdrecht, Netherlands; International Astronomical Union symposium no. 93 on fundamental problems in the theory of stellar evolution; Kyoto, Japan; 22 - 25 Jul 1980; 50 refs.