The Synthesis of Helium and CNO Isotopes in Massive Stars

Details The Synthesis of Helium and CNO Isotopes in Massive Stars The Synthesis of Helium and CNO Isotopes in Massive Stars

Nov 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ssrv...74..343l&link_type=abstract

Space Science Reviews, Volume 74, Issue 3-4, pp. 343-353

Physics

33

Stellar Evolution, Nucleosynthesis, Mass Loss, Supernovae, Chemical Evolution

Scientific paper

We present helium and CNO isotopic yields for massive mass-losing stars
in the initial mass range 15M &sun; ≤M i ≤
50M &sun;. We investigate their dependence on assumptions
about mass loss rates, internal mixing processes, and metallicity, and
specify the contributions from stellar winds and from supernova ejecta.

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