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Tachocline mixing, light elements in halo stars

Published online by Cambridge University Press:  23 December 2005

Laurent Piau
Laurent Piau
Affiliation:
University of Chicago, 933, East 56th Street, Chicago, IL, 60637, USA email: piau@oddjob.uchicago.edu
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Abstract

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We have computed updated models of population II stars on the Spite plateau. We focus here on the light elements abundance predictions when the new tachocline mixing process is accounted for.

Keywords

Stars: interiorsstars: abundancesstars: rotation
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. 107 - 108
Copyright
© 2005 International Astronomical Union