On the Origin of Emission in the White-Light Continuum in Powerful Stellar and Solar Flares
摘要
In this study, attention is drawn to some observable manifestations of the existence of two separate regions with different temporal development during powerful flares on dMe stars and on the Sun. I propose a theoretical interpretation of the origin of the white-light continuum in powerful stellar flares with classical light curves and discuss it in the context of observations of the white-light flares of the first type on the Sun.