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- W2001110045 abstract "A star is considered to consist of two zones, one of which contains a nuclear source. The interaction between the two zones can lead to slow oscillations during which the star remains near hydrostatic equilibium. The model permits a discussion of the roles played by thermonuclear reactions, radiative heat transport, and hydrostatic adjustment to heat input. Applications are made to stars on the main sequence and to stars with helium-burning shells. (auth)" @default.
- W2001110045 created "2016-06-24" @default.
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- W2001110045 date "1973-05-01" @default.
- W2001110045 modified "2023-09-25" @default.
- W2001110045 title "A Simplified Model for Oscillatory Secular Modes" @default.
- W2001110045 doi "https://doi.org/10.1086/152132" @default.
- W2001110045 hasPublicationYear "1973" @default.
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