evelite

这颗明亮的蓝色恒星属于恒星风及其猛烈而且旋转迅速的那一种类型。他们的大部分能量产生于其质量中心，通过包括了碳-氮-氧（CNO）催化循环的热核聚变过程而来。这种类型的恒星会发出强烈的非电离氦线条，有些还会因化学反应而放出及其强烈的线条，由此得名为“强氦星”。

This luminous blue star belongs to a class known for powerful stellar winds and rapid rotation. These stars generate most of their energy at the center of their mass in a thermonuclear fusion process involving a carbon-nitrogen-oxygen (CNO) catalytic cycle. Stars of this type generally show strong non-ionized helium lines and some have a chemistry that results in very strong lines, leading to the designation 'helium-strong'.