摘要
恒星之一生,长者可达几万亿年,短则不到一千万年,期间历经多次短时标的灾变事件,而此类事件出现前后,恒星多方面性质发生了非常剧烈的、甚至是根本性的改变。对此,天文学家已经有了较为充分的认识,但尚未完全洞悉其中之众多奥秘。
It is briefly introduced in this paper how white dwarfs, neutron stars or black holes can be finally produced through col- lapse process of cvolvcd stars with different masses, and what are the main physical and structural characteristics of these kinds of ce- lestial compact objects. Besides, some serious influences of stellar catastrophes on our planet, the earth, and human being lived on it that will probably occur in future are discussed.
出处
《自然杂志》
北大核心
2010年第5期255-259,共5页
Chinese Journal of Nature
关键词
行星状星云
白矮星
中子星
黑洞
planetary nebula, white dwarf, neutron star, black hole