Giovedì 20 marzo alle ore 15:00, il Dr. Patrick Eggenberger dell’Università di Ginevra (Svizzera) terrà il seminario dal titolo “Stellar evolution with rotation and magnetic fields”.

Abstract
Stellar physics connects fundamental physical aspects to hydrodynamic and magnetohydrodynamic processes, and the validity of stellar models depends directly on our understanding of these physical mechanisms. In this talk, we will first discuss how asteroseismology, the study of stellar oscillations, can help us progress in the modelling of angular momentum and chemicals transport in stellar interiors. We will then describe the impact of these transport processes on the evolution of stars.