The impact of rotation on the stochastic excitation of stellar acoustic modes in solar-like pulsators
Context. Recent observational results from asteroseismic studies show that an important fraction of solar-like stars do not present detectable stochastically excited acoustic oscillations. This non-detectability seems to correlate with a high rotation rate in the convective envelope and a high surface magnetic activity. At the same time, the
Bessila, L. et al.
Fecha de publicación:
8
2025