论文标题
在DME恒星的弹性阶段的光辐射的起源上。 ii。连续辐射
On the Origin of Optical Radiation During the Impulsive Phase of Flares on dMe Stars. II. Continuum and Line Radiation
论文作者
论文摘要
有人认为，不仅蓝色（最大亮度最大），而且还形成了DME恒星上功能强大弹性的光连续体的红色（在慢速衰减阶段）成分，在光球附近形成。注意到，由于电子与原子和离子的弹性碰撞而导致电子温度升高，HEI线的可能出现在血浆的弛豫区域中的可能出现（由于原子和离子的弹性碰撞而导致的）（对于非稳态的彩色冲击速度的高速高速，朝着太阳和星星的照片传播的照片）。提出了一种方案，用于在强大的恒星耀斑的冲动阶段的白光连续体中产生辐射的“层”的定位。
It is argued that not only the blue (at the brightness maximum) but also the red (in the slow decay phase) components of the optical continuum of powerful flares on dMe stars are formed near the photosphere. The possible appearance of HeI lines in the relaxation zones for the plasma to a state of thermal equilibrium (as a result of a rise in electron temperature owing to elastic collisions of electrons with atoms and ions) is noted (for sufficiently high speeds of a non-stationary chromospheric shock wave propagating toward the photosphere of the Sun and stars). A scheme is proposed for the positioning of the "layers" of plasma responsible for the generation of radiation in the white light continuum during the impulsive phase of powerful stellar flares.
