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Massive stars: stellar models and stellar yields, impact on Galactic Archaeology

Published online by Cambridge University Press:  02 August 2018

Georges Meynet ,
Arthur Choplin ,
Sylvia Ekström Open the ORCID record for Sylvia Ekström [Opens in a new window]  and
Cyril Georgy Open the ORCID record for Cyril Georgy [Opens in a new window]
Georges Meynet
Affiliation:
Department of Astronomy, University of Geneva, CH-1290 Versoix, Switzerland email: georges.meynet@unige.ch
Arthur Choplin
Affiliation:
Department of Astronomy, University of Geneva, CH-1290 Versoix, Switzerland email: georges.meynet@unige.ch
Sylvia Ekström
Affiliation:
Department of Astronomy, University of Geneva, CH-1290 Versoix, Switzerland email: georges.meynet@unige.ch
Cyril Georgy
Affiliation:
Department of Astronomy, University of Geneva, CH-1290 Versoix, Switzerland email: georges.meynet@unige.ch
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Abstract

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The physics of massive stars depends (at least) on convection, mass loss by stellar winds, rotation, magnetic fields and multiplicity. We briefly discuss the impact of the first three processes on the stellar yields trying to identify some guidelines for future works.

Keywords

StarsnucleosynthesiswindsrotationsupernovaeyieldsCEMP stars
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 13 , Symposium S334: Rediscovering our Galaxy , July 2017 , pp. 170 - 177
Copyright
Copyright © International Astronomical Union 2018 

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