Unveiling structures in the evolution of magnetic activity of solar-like stars
The magnetic and rotational properties of solar-like stars are strongly coupled due to the interaction of rotation and convection in their outer envelopes, which fuels their magnetic dynamos and, as a consequence, their magnetic activity cycles. Thanks to the large number of Kepler targets with measured rotation periods and photometric magnetic
Mathur, Savita et al.
Fecha de publicación:
8
2024