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Angular Momentum Evolution of Young Solar-type Stars

Published online by Cambridge University Press:  27 January 2016

Louis Amard ,
Ana Palacios  and
Corinne Charbonnel
Louis Amard
Affiliation:
LUPM, Université Montpellier, CNRS, Place Eugène Bataillon, 34095 MontpellierFrance email: louis.amard@univ-montp2.fr Geneva Observatory, University of Geneva, Chemin des Maillettes, 51, 1290 Versoix, Switzerland
Ana Palacios
Affiliation:
LUPM, Université Montpellier, CNRS, Place Eugène Bataillon, 34095 MontpellierFrance email: louis.amard@univ-montp2.fr
Corinne Charbonnel
Affiliation:
Geneva Observatory, University of Geneva, Chemin des Maillettes, 51, 1290 Versoix, Switzerland IRAP departement of astronomy, CNRS UMR 5277, Université de Toulouse, 14, Av. E.Belin, 31400 Toulouse, France
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Abstract

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We present stellar evolution models of young solar-type stars including self consistent treatment of rotational mixing and extraction of angular momentum (AM) by magnetized wind including the most up-to-date physic of AM transport.

Keywords

stars: evolutionstars: rotationstars: wind-brakinghydrodynamics

Information

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 10 , Issue S314: Young Stars & Planets Near the Sun , November 2015 , pp. 109 - 112
Copyright
Copyright © International Astronomical Union 2016 

References

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