Final Stages of Stellar Evolution and Nucleosynthesis: What do We Know and What Would We Like to Know?

Details Final Stages of Stellar Evolution and Nucleosynthesis: What do We Know and What Would We Like to Know? Final Stages of Stellar Evolution and Nucleosynthesis: What do We Know and What Would We Like to Know?

Jul 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002ap%26ss.281..173h&link_type=abstract

Astrophysics and Space Science, v. 281, Issue 1, p. 173-182 (2002).

Astronomy and Astrophysics

Astrophysics

Supernovae, Nucleosynthesis

Scientific paper

Recent developments in theoretical model-calculations for the synthesis of the chemical elements during late stages of stellar evolution are reviewed. Special emphasis is put on a discussion of various astrophysical sites, including core-collapse and thermonuclear supernovae, and the physics of turbulent reactive fluids. Results of numerical simulations are presented and discussed, together with new results concerning solar-system abundances as well as abundances observed in very metal-poor stars, in the context of searches for constraints on the still rather uncertain nuclear physics data and astrophysical models.

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