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Fast rotating first stars

Published online by Cambridge University Press:  23 December 2005

Sylvia Ekström ,
Georges Meynet  and
André Maeder
Sylvia Ekström
Affiliation:
Geneva Observatory, Maillettes 51, CH - 1290 Sauverny, Switzerland, email: sylvia.ekstrom@obs.unige.ch
Georges Meynet
Affiliation:
Geneva Observatory, Maillettes 51, CH - 1290 Sauverny, Switzerland, email: sylvia.ekstrom@obs.unige.ch
André Maeder
Affiliation:
Geneva Observatory, Maillettes 51, CH - 1290 Sauverny, Switzerland, email: sylvia.ekstrom@obs.unige.ch
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Abstract

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In order to study the effects of fast rotation on primordial stars, we present the evolution and the chemical yields of zero metallicity models with masses between 15 to 200 M[odot ].

Keywords

Stars: abundancesstars: rotationearly universe
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 1 , Symposium S228: From Lithium to Uranium: Elemental Tracers of Early Cosmic Evolution , May 2005 , pp. 163 - 164
Copyright
© 2005 International Astronomical Union