Observational Constraints on Nucleosynthesis and Mixing in AGB Stars

Details Observational Constraints on Nucleosynthesis and Mixing in AGB Stars Observational Constraints on Nucleosynthesis and Mixing in AGB Stars

Sep 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011aspc..445...13a&link_type=abstract

Why Galaxies Care about AGB Stars II: Shining Examples and Common Inhabitants. Proceedings of a conference held at University Ca

Astronomy and Astrophysics

Astronomy

Scientific paper

AGB stars are excellent laboratories to investigate the nucleosynthesis and mixing processes occurring during the later phases of the evolution of low and intermediate mass stars. The determination of the abundances of several key elements in their atmospheres - such as Li, CNO and their isotopic ratios, fluorine, s-elements, etc. - is a key tool to constrain theoretical AGB models. In this contribution, I briefly discuss some recent results and current problems on this subject.

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