Speaker
Allan Sacha Brun
(Laboratoire AIM Paris-Saclay, CEA/Irfu Université Paris)
Description
We will present our recent efforts to model G & K stars with the ASH code. We have
designed new model coupling the convective envelope to a deep stable radiative
interior. We have varied both the mass & rotation rates in order to pave a large
parameter space and to derive scaling laws for these type of solar-like stars. We
have also introduced seed magnetic field to study how dynamo action is influenced by
the underlying stellar structure and rotation rate.
Primary authors
Allan Sacha Brun
(Laboratoire AIM Paris-Saclay, CEA/Irfu Université Paris)
Olivier Do Cao
(Laboratoire AIM Paris-Saclay, CEA/Irfu Université Paris)
Sean P. Matt
(Laboratoire AIM Paris-Saclay, CEA/Irfu Université Paris)
