Presolar SiC Grains and Rare Earth Element Production in AGB Stars

Details Presolar SiC Grains and Rare Earth Element Production in AGB Stars Presolar SiC Grains and Rare Earth Element Production in AGB Stars

Apr 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aipc.1001..237d&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

Giant And Subgiant Stars, Stellar Structure, Interiors, Evolution, Nucleosynthesis, Ages, Abundances, Chemical Composition

Scientific paper

The relative abundances of many isotopes of the rare earth elements are
strongly affected by s-process nucleosynthesis in low-mass asymptotic
giant branch (AGB) stars. We briefly explore the nucleosynthesis of the
rare earth elements in AGB stars and their implications for measurements
of presolar SiC grains from those stars.

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