Constraining the core-rotation rate along the red-giant evolution
The evolution of the core rotation rate of red giant stars is a key parameter in understanding the stellar behavior in the late phases of stellar evolution. Thanks to the mixed-dipole modes, we can constrain the core rotation and internal rotational gradient as a star advances through the red-giant phase. This master thesis presents a pipeline
Muntean, N. et al.
Fecha de publicación:
3
2024