Yields from single AGB stars

Details Yields from single AGB stars Yields from single AGB stars

2007-08-29

arxiv.org/abs/0708.4020v1

Astronomy and Astrophysics

Astrophysics

8 pages. To appear in "Asymmetrical Planetary Nebulae IV," eds. R. L. M. Corradi, A. Manchado & N. Soker

Scientific paper

In order to understand the composition of planetary nebulae we first need to study the nucleosynthesis occurring in the progenitor star during the thermally-pulsing Asymptotic Giant Branch (AGB) phase. I present an overview of single AGB evolution, with an emphasis on the mixing processes that alter the envelope composition, followed by a discussion of the stellar yields available from single AGB stellar models.

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