s-Process Enhancement During the AGB Phase

Details s-Process Enhancement During the AGB Phase s-Process Enhancement During the AGB Phase

Apr 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aipc.1001..213w&link_type=abstract

IXTH TORINO WORKSHOP ON EVOLUTION AND NUCLEOSYNTHESIS IN AGB STARS AND THE IIND PERUGIA WORKSHOP ON NUCLEAR ASTROPHYSICS. AIP C

Astronomy and Astrophysics

Astrophysics

Carbon Stars, S Stars, And Related Types, Abundances, Chemical Composition, Stellar Structure, Interiors, Evolution, Nucleosynthesis, Ages

Scientific paper

The results of a study of the AGB phase are presented. Abundances have been determined for Fe, C, O, the light s-process elements, Y and Zr, the heavy s-process elements, La and Nd, and the r-process element, Eu. The expected relationship between enhanced C, increasing C/O ratio and enhanced s-process elements has been quantified. Results are presented to provide observational data with which to compare theoretical predictions. This paper gives a brief overview of results, full details of the analysis and thorough discussion can be found in Wylie de Boer and Cottrell, 2008 [1].

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