S Process Noble Gases in Meteorites and their Astrophysical Origin

Details S Process Noble Gases in Meteorites and their Astrophysical Origin S Process Noble Gases in Meteorites and their Astrophysical Origin

Apr 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003eaeja....13779f&link_type=abstract

EGS - AGU - EUG Joint Assembly, Abstracts from the meeting held in Nice, France, 6 - 11 April 2003, abstract #13779

Astronomy and Astrophysics

Astrophysics

Scientific paper

An updated analysis of the astrophysical origin of nobles gas components
carried by presolar SiC grains is discussed. New stellar evolutionary
models have been followed, together with updated network of neutron
capture cross sections. Results for Ne, Kr and Xe are presented.

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