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| | Analysis of Stellar Atmospheres and Pulsation
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| | Our research is focussing on a better understanding of the photosphere and internal structure of stars with an evolutionary status ranging from pre main sequence to core hydrogen burning. We work on theory and interprete observational data produced on ground and in space.
A.S.A.P. is a successor to the project Asteroseismology along the Main Sequence | | |
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