传统的星系演化模型之一预言，宇宙早期的小星系通过结合演化成大质量的星系。
One of the conventional models for galaxy evolution predicts that small galaxies in the early Universe evolved into the massive galaxies of today by coalescing.
他们的新模型再现了130亿年的宇宙演化史，得到的结果与我们今天所看到的各种不同星系惊人的吻合。
Their new model reproduces 13 billion years? Worth of cosmic evolution, resulting in a surprisingly accurate tally of the different kinds of galaxies we see.
他们的新模型再现了130亿年的宇宙演化史，得到的结果与我们今天所看到的各种不同星系惊人的吻合。
Their new model reproduces 13 billion years' worth of cosmic evolution, resulting in a surprisingly accurate tally of the different kinds of galaxies we see.
利用描述引力系统演化的伏拉索夫方程的标度关系探讨了宇宙中星系团分布的一些标度律，并结合一个宇宙加速模型进行了讨论。
A new scaling analysis to the Vlasov equation which describes gravitational clustering is performed, and then it is argued with universe accelerative expanse modal.
然而在大爆炸宇宙模型和恒星演化理论之间存在一个人们了解甚少的领域：就是由大量恒星组成而又作为宇宙基本单元的星系是如何形成和演化的?。
Between the theories of big-bang cosmology and the theory of stellar structure and theory, there is a gap still rarely understood: how do the galaxies form?
本模型以银河系球状星团的形成和演化为出发点，但同样普适于其它星系中球状星团的形成和演化。
It is shown as well that this model is successful to apply not only to GCs in our Galaxy, but also to those in other galaxies as they have a universal formation process.
本模型以银河系球状星团的形成和演化为出发点，但同样普适于其它星系中球状星团的形成和演化。
It is shown as well that this model is successful to apply not only to GCs in our Galaxy, but also to those in other galaxies as they have a universal formation process.
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