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Fluorine Production from AGB and WR Stars

Published online by Cambridge University Press:  19 July 2016

Nami Mowlavi  and
Georges Meynet
Nami Mowlavi
Affiliation:
Geneva Observatory CH-1290 Sauverny, Switzerland
Georges Meynet
Affiliation:
Geneva Observatory CH-1290 Sauverny, Switzerland

Abstract

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The role of Wolf-Rayet and asymptotic giant branch stars in the production of the Solar System fluorine abundance is analyzed. It is shown that both these stars can be important sources of galactic fluorine. However, the uncertainties affecting the predictions, especially those from asymptotic giant branch stars, do not allow to give quantitative figures yet.

Type
Conference Papers in order of Presentation
Information
Symposium - International Astronomical Union , Volume 187: Cosmic Chemical Evolution , 2002 , pp. 71 - 73
Copyright
Copyright © 2002 

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