Core─Envelope Coupling in Intermediate-mass Core-helium Burning Stars
Stars between two and three solar masses rotate rapidly on the main sequence, and the detection of slow core and surface rotation in the core-helium burning phase for these stars places strong constraints on their angular momentum transport and loss. From a detailed asteroseismic study of the mixed-dipole mode pattern in a carefully selected
Tayar, Jamie et al.
Fecha de publicación:
12
2019