The Late Evolution of WC Stars: Weak S-Process and Neutron-Rich Nuclei in Cosmic Rays

Details The Late Evolution of WC Stars: Weak S-Process and Neutron-Rich Nuclei in Cosmic Rays The Late Evolution of WC Stars: Weak S-Process and Neutron-Rich Nuclei in Cosmic Rays

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983icrc....9..155p&link_type=abstract

Proceedings from the 18th International Cosmic Ray Conference, held in Bangalore, India, 22 August - 3 September, 1983. Volume

Physics

Scientific paper

The authors reexamine and extend the study of nucleosynthesis in the
most massive WC stars, since this unique class of objects seems to offer
a natural explanation for the 12C, 22Ne,
25Mg and 26Mg excesses inferred at the cosmic-ray
sources w.r.t. solar system.

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