Speaker
Prof.
Raphael Hirschi
(Keele University )
Description
Stars are complex three-dimensional (3D) objects involving many physical processes: convection, rotation, magnetic fields. In this talk, I will review the efforts to constrain the physical ingredients of 1D stellar evolution models of the first stars using multi-D (magneto-)hydrodynamic simulations.
Primary author
Prof.
Raphael Hirschi
(Keele University )
