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Nucleosynthesis in Red Giant Stars

Published online by Cambridge University Press:  19 July 2016

Nami Mowlavi
Nami Mowlavi*
Affiliation:
Geneva Observatory CH-1290 Sauverny, Switzerland

Abstract

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The production of elements from helium-3 to fluorine in low- and intermediate-mass stars is reviewed and compared to chemical abundances observed at the surface of both red giant branch and asymptotic giant branch stars. It is highlighted that, while the trends predicted by standard models are generally well confirmed, many chemical abundances observed at the surface of red giants require the operation of non-standard mixing in the stellar interior. In addition, chemical abundance predictions from presently available asymptotic giant branch models further suffer from the uncertainties affecting the third dredge-up phenomenon, the source of neutrons and the hot bottom burning process.

Type
Conference Papers in order of Presentation
Information
Symposium - International Astronomical Union , Volume 187: Cosmic Chemical Evolution , 2002 , pp. 57 - 69
Copyright
Copyright © 2002 

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