Modeling The Nucleosynthesis Of Massive Stars

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This overview discusses issues relevant to modeling nucleosynthesis in type II supernovae and implications of detailed studies of the ejecta. After a brief presentation of the most common approaches to stellar evolution and parameterized explosions, the relevance of a number of nuclei to obtain information on the evolution and explosion mechanisms is discussed. The paper is concluded by an outlook on multi-dimensional simulations.
Invited talk at the workshop "Astronomy with Radioactivities IV", Seeon, Germany, June 2003; 6 pages, to appear in New Astronomy Reviews

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Astrophysics

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http://salesiana.dossiersoluciones.com/handle/123456789/6454

Consulte el texto completo en el siguiente enlace:

https://arxiv.org/abs/astro-ph/0309262
 http://arxiv.org/abs/astro-ph/0309262
 New Astron.Rev. 48 (2004) 3
 doi:10.1016/j.newar.2003.11.002

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arXiv