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Nucleosynthesis in AGB Stars

Published online by Cambridge University Press:  25 May 2016

John Lattanzio  and
Manuel Forestini
John Lattanzio
Affiliation:
Dept of Mathematics and Statistics, Monash University, Australia Institute of Astronomy, Madingley Rd, Cambridge, England
Manuel Forestini
Affiliation:
Laboratoire d'Astrophysique, Université Joseph Fourier, Grenoble, France

Abstract

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We give a qualitative review of the nucleosynthesis occurring in AGB stars. We summarise some new calculations of intermediate mass stars which include all thermal pulses until the star is about to leave the AGB, as well as a detailed nucleosynthesis network. We will show that hot bottom burning delays, rather than prevents, the formation of carbon stars; those that form are not optically visible.

Type
Part 1. Basic Facts, Structure, Evolution, Nucleosynthesis
Information
Symposium - International Astronomical Union , Volume 191: Asymptotic Giant Branch Stars , 1999 , pp. 31 - 40
Copyright
Copyright © Astronomical Society of the Pacific 1999 

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