Daniel Huber
Published 2014-11-04Version 1
The measurement of oscillations excited by surface convection is a powerful method to study the structure and evolution of cool stars. CoRoT and Kepler have initiated a revolution in asteroseismology by detecting oscillations in thousands of stars from the main sequence to the red-giant branch, including a large number of exoplanet host stars. In this contribution I will review recent asteroseismic results, focusing in particular on the internal rotation of red giant stars and the impact of asteroseismology on the characterization of exoplanets.
Comments: 13 pages, 7 figures; Proceedings of the 18th Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun, Eds G. van Belle & H. Harris
Asteroseismology of red giant stars: the potential of dipole modes
Asteroseismology of Exoplanet-Host Stars in the Kepler Era
Asteroseismology of 19 low-luminosity red giant stars from Kepler
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