Projects
The TOS group as a whole focusses on the understanding of stellar structure and evolution of predominantly low-mass stars. This is done in a holistic way using different kinds of observations (spectroscopy, photometry, asteroseismology, astrometry and when available interferometry) and stellar models. In short we are on “the quest for the ultimate stellar model”.
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SFB 881 ‘Milky Way galaxy: Asteroseismic stellar parameters of open cluster stars’
The goals of this project are the following: – an in-depth characterization of the three Kepler open clusters (NGC 6791, 6811 and 6819) to …
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ERC consolidator grant ‘DipolarSound’
The aim of the DipolarSound proposal is to unravel the physical conditions and physical processes at play in red-giant stars using …
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