Temporal variation of the photometric magnetic activity for the Sun and Kepler solar-like stars
Context. The photometric time series of solar-like stars can exhibit rotational modulation, that is, brightness variations due to active regions co-rotating with the stellar surface. These signatures allow us to constrain properties of stellar rotation and magnetic activity. Aims: In this work we investigate the behavior, particularly the
Santos, A. R. G. et al.
Fecha de publicación:
4
2023