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- W1556891489 abstract "The x‐ray burst phenomenon is interpreted in terms of a nuclear shell flash on the surface of an accreting neutron star. The thermal and nuclear evolution of the envelope is described for the hydrogen‐helium shell flash and the nearly pure helium shell flash cases. The differences between shell flash modes are discussed and compared with the average properties of x‐ray bursts. Several outstanding problems that remain for the thermonuclear flash model are listed and possible resolutions are suggested." @default.
- W1556891489 created "2016-06-24" @default.
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- W1556891489 date "1984-01-01" @default.
- W1556891489 modified "2023-10-17" @default.
- W1556891489 title "The thermonuclear flash model for X-ray bursts" @default.
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- W1556891489 doi "https://doi.org/10.1063/1.34530" @default.
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