Nucleosynthesis in massive stars revisited

Details Nucleosynthesis in massive stars revisited Nucleosynthesis in massive stars revisited

2000-10-02

arxiv.org/abs/astro-ph/0010021v1

Nucl. Phys. A688 (2001) 193

Astronomy and Astrophysics

Astrophysics

4 pages, 1 figure; needs espcrc1.sty; talk at "Nuclei in the Cosmos 2000", Aarhus, Denmark, June 2000; will appear in Nucl. Ph

Scientific paper

10.1016/S0375-9474(01)00696-0

We have performed the first calculations to follow the evolution of all stable nuclei and their radioactive progenitors in a finely-zoned stellar model computed from the onset of central hydrogen burning through explosion as a Type II supernova. Calculations were done for 15, 20, and 25 solar masses Pop I stars using the most recently available set of experimental and theoretical nuclear data, revised opacity tables, and taking into account mass loss due to stellar winds. Here results are presented for one 15 solar masses model.

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