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星系形成和演化
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作者 莫厚俊 《天文学进展》 CSCD 北大核心 2001年第2期112-112,共1页
在现代宇宙学的框架下对当前星系形成和演化方面的研究结果作一综合评述.内容包括各种现代化观测手段所得的结果及其物理内涵、各种模型的成功与不足之处。
关键词 星系形成 星系演化 宇宙学模型 现代宇宙学
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SECONDARY EFFECTS OF COSMIC STRING
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作者 莫厚俊 《Science China Mathematics》 SCIE 1989年第3期328-337,共10页
The reionization and the large-scale structure formation of the universe are consi-dered as results of the secondary effects of cosmic string. Primordial supermassive (~10~6M_⊙) stars and star groups M(~10^(10)M_⊙... The reionization and the large-scale structure formation of the universe are consi-dered as results of the secondary effects of cosmic string. Primordial supermassive (~10~6M_⊙) stars and star groups M(~10^(10)M_⊙) can be formed immediately after recombinationowning to the accretions of single-string loops. The ultraviolet radiation of the starscan reionize the interstellar medium around them. The explosions of the supermassivestars sweep the interstellar medium to the shock-wave front to form mass shells of largemass and high density; the fragmentations of the mass shells lead to formations of newstars and new explosions. It is shown, when Grand Unification Theory (GUT) stringsare taken to be the seeds, the observed high ionization and large-scale cellular structureof galaxy distribution in the universe can be realized. For the usually chosen parameters,this scenario seems reasonable and imperative. 展开更多
关键词 COSMIC string.
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