Hostname: page-component-586b7cd67f-t8hqh Total loading time: 0 Render date: 2024-11-20T17:42:46.228Z Has data issue: false hasContentIssue false
  • English
  • Français

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: [email protected]
Georges Meynet
Affiliation:
Geneva Observatory, Maillettes 51, CH - 1290 Sauverny, Switzerland, email: [email protected]
André Maeder
Affiliation:
Geneva Observatory, Maillettes 51, CH - 1290 Sauverny, Switzerland, email: [email protected]
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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