CORDIS Project
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This project investigates the evolution of low- and intermediate-mass stars in the Milky Way, focusing on the effects of rotation and mixing on their chemical composition. The applicant will utilize asteroseismology to enhance understanding of stellar evolution.
Low- and intermediate-mass stars form the dominant stellar component of our Galaxy and represent a very important astrophysical interest.
Their location, kinetics and chemistry give informations on the mechanism of the formation and evolution of the Milky Way.
During her PhD thesis, the applicant showed the crucial role of rotation-induced mixing and thermohaline instability to better understand the chemical evolution of red giant stars, and their consequences on the evolution of light elements…
THE UNIVERSITY OF BIRMINGHAM
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