Invited comunication
M. S. Cunha
Abstract
Intermediate-mass stars stand out as unique
physics laboratories due to the diversity and
range of physical phenomena they exhibit.
With rotation spanning from extremely
slow to fast, a chemical composition that
ranges from highly peculiar to normal,
and magnetic fields varying from very
strong to undetectable, these stars provide
exceptional conditions for advancing our
studies in crucial aspects of stellar physics.
Exploring these stars further contributes to
enhancing our models of stellar evolution.
In this presentation, I will delve into recent
findings from studies of intermediate-mass
stars and address the key challenges they
continue to present.
Crafoord Days 2024
Stockholm, Sweden
2024 May
