Detailed cool star flare morphology with CHEOPS and TESS***
Context. White-light stellar flares are proxies for some of the most energetic types of flares, but their triggering mechanism is still poorly understood. As they are associated with strong X and ultraviolet emission, their study is particularly relevant to estimate the amount of high-energy irradiation onto the atmospheres of exoplanets
Alonso, R. et al.
Fecha de publicación:
6
2024