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Transport of angular momentum in solar-like oscillating stars

Published online by Cambridge University Press:  18 February 2014

Mariejo Goupil ,
Sébastien Deheuvels ,
Joao Marques ,
Yveline Lebreton ,
Benoit Mosser ,
Rafa García ,
Kevin Belkacem  and
Stéphane Mathis
Mariejo Goupil
Affiliation:
Observatoire de Paris, LESIA, CNRS UMR 8109, F-92190 Meudon, France email: [email protected]
Sébastien Deheuvels
Affiliation:
Université de Toulouse, UPS-OMP IRAP, CNRS, F-31400 Toulouse, France
Joao Marques
Affiliation:
Institut d'Astrophysique Spatiale, UMR 8617, CNRS, Université Paris XI, 91405 Orsay Cedex, France
Yveline Lebreton
Affiliation:
Observatoire de Paris, GEPI, CNRS UMR 8109, F-92190 Meudon, France Institut de Physique de Rennes, Université de Rennes 1, CNRS UMR 6251, F-35042 Rennes, France
Benoit Mosser
Affiliation:
Observatoire de Paris, LESIA, CNRS UMR 8109, F-92190 Meudon, France email: [email protected]
Rafa García
Affiliation:
Laboratoire AIM Paris-Saclay, CEA/DSM-CNRS-Université Paris Diderot, IRFU/SAp Centre de Saclay, 91191 Gif-sur-Yvette, France
Kevin Belkacem
Affiliation:
Observatoire de Paris, LESIA, CNRS UMR 8109, F-92190 Meudon, France email: [email protected]
Stéphane Mathis
Affiliation:
Laboratoire AIM Paris-Saclay, CEA/DSM-CNRS-Université Paris Diderot, IRFU/SAp Centre de Saclay, 91191 Gif-sur-Yvette, France
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Abstract

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Our current understanding and modeling of angular momentum transport in low-mass stars are briefly reviewed. Emphasis is set on single stars slightly younger that the Sun and on subgiants and red giants observed by the space missions CoRoT and Kepler.

Keywords

stars: solar-typestars: oscillationsstars: rotationstars: evolutionstars: interiors
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 9 , Symposium S301: Precision Asteroseismology , August 2013 , pp. 161 - 168
Copyright
Copyright © International Astronomical Union 2014 

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