Internal rotation of red giants by asteroseismology
1 INAF-IAPS Roma, Italy
2 INAF-Osservatorio Astrofisico di Catania, Italy
3 Sydney Institute for Astronomy, School of Physics, University of Sydney, Australia
4 Instituut voor Sterrenkunde, Katholieke Universiteit Leuven, Belgium
5 AIM, CEA/DSM-CNRS-Université Paris Diderot, IRFU/Sap., Centre de Saclay, France
6 School of Physics and Astronomy, University of Birmingam, UK
7 Astronomical Institute Anton Pannekoek, University of Amsterdam, The Netherlands
8 LESLIA, CNRS, Université Pierre et Marie Curie, Université Denis Diderot, Observatoire de Paris, Meudon Cedex, France
9 Department of Physics and Astronomy, Aarhus University, Denmark
a e-mail: email@example.com
We present an asteroseismic approach to study the dynamics of the stellar interior in red giant stars by asteroseismic inversion of the splittings induced by the stellar rotation on the oscillation frequencies. We show preliminary results obtained for the red giant KIC4448777 observed by the space mission Kepler.
© Owned by the authors, published by EDP Sciences, 2013
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