The Influence of Mass Loss on the Evolution and Nucleosynthesis of Massive Stars

Details The Influence of Mass Loss on the Evolution and Nucleosynthesis of Massive Stars The Influence of Mass Loss on the Evolution and Nucleosynthesis of Massive Stars

Apr 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aipc.1001...19c&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

Stellar Structure, Interiors, Evolution, Nucleosynthesis, Ages, Abundances, Chemical Composition, Main-Sequence: Early-Type Stars, Supernovae, Mass Loss And Stellar Winds

Scientific paper

We briefly discuss the influence of mass loss on the internal
evolutionary properties of massive stars. In particular we show that the
C abundance left by the central He burning depends significantly on the
adopted mass loss rate after the H rich mantle has been completely
ejected.

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