Asteroseismology of red giant stars: The potential of dipole modes
Université de Liège, Allée du Six Août -17, 4000 Liège, Belgium
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Since the detection of non-radial solar-like oscillation modes in red giants with the CoRoT satellite, the interest in the asteroseismic properties of red giants and the link with their global properties and internal structure is increasing. Moreover, more and more precise data are being collected with the space-based telescopes CoRoT and Kepler. Particularly relevant has been the detection of mixed modes in a large number of G-K red giants. In this contribution we discuss the potential of these dipole mixed modes to provide information on core extra-mixing and transport of angular momentum.
© Owned by the authors, published by EDP Sciences, 2013
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