Computing Cool Bottom Process Effects in Low Mass AGB Stars

Details Computing Cool Bottom Process Effects in Low Mass AGB Stars Computing Cool Bottom Process Effects in Low Mass AGB Stars

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1213..228p&link_type=abstract

FIFTH EUROPEAN SUMMER SCHOOL ON EXPERIMENTAL NUCLEAR ASTROPHYSICS. AIP Conference Proceedings, Volume 1213, pp. 228-231 (2010).

Astronomy and Astrophysics

Astrophysics

1

Stellar Evolution, Nucleosynthesis, Stellar Mass, Stellar Magnetism, Black Holes, Stellar Structure, Interiors, Evolution, Nucleosynthesis, Ages, Masses, Interplanetary Magnetic Fields

Scientific paper

Isotopic ratios of C, N and O not in agreement with the canonical stellar evolutionary models are shown by spectra of evolved low mass stars and by presolar grains formed in their circumstellar origin. It has been shown in literature that partial mixing between the inner stellar regions and the base of the convective envelope can produce these chemical anomalies. We briefly describe how the evolution composition induced by such mixing episodes can be computed.

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