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- W88628708 abstract "An attempt is reported to build self-consistent evolutionary models of complete massive stars, starting from their observable zero-age main sequence configurations, and evolving through their various hydrostatic nuclear burning stages, iron core collapse, bounce, outward-going shock formation, and finally, explosive nucleosynthesis and supernovae light curve formation. The model incorporates implicit hydrodynamics with a new treatment of time-dependent convection and semiconvection, and a careful treatment of the complexities of the advanced stages of stellar burning. The model was used to completely evolve population I stars of 15 and 25 M/sub solar mass/, with excellent agreement with the known properties and the prediction of other properties. 65 references. (JFP)" @default.
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- W88628708 date "1978-12-01" @default.
- W88628708 modified "2023-09-23" @default.
- W88628708 title "Evolution and explosion of massive stars. [Hydrodynamics, convection]" @default.
- W88628708 hasPublicationYear "1978" @default.
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