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The MAMSIE project focuses on developing advanced models of massive stars by analyzing gravity-mode oscillations. It aims to enhance our understanding of stellar structure and evolution through a data-driven approach, integrating insights from hydrodynamics and seismic observations.
With the CoRoT & Kepler data analysed, the time is optimal to move from observational asteroseismology to innovative stellar modelling of the steal factories of the Universe.
With MAMSIE, we follow the footsteps of helioseismologists some 30 years after them, but this time we shall be developing inversion methods for stellar structure based on gravity-mode oscillations that probe the deep stellar interior. MAMSIE will lead to new models for a variety of single and binary stars with masses betwee…
KATHOLIEKE UNIVERSITEIT LEUVEN
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