中央研究院天文及天文物理研究所 Institute of Astronomy and Astrophysics, Academia Sinica
大質量恆星在演化的後期，其核心常會發生不穩定的核融合反應，導致劇烈的物質噴發。
In the later stages of evolution, massive stars often experience unstable nuclear fusion reactions in their cores, leading to violent ejections of matter.
