Fragmentation of the Primordial Gas Clouds and the Lower Limit on the Mass of the First Stars

Fragmentation of the Primordial Gas Clouds and the Lower Limit on the Mass of the First Stars
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原始气体云的破碎和第一颗恒星质量的下限

DOI:
10.1086/310409
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发表时间:
1996
期刊:
The Astrophysical Journal Letters
影响因子:
--
通讯作者:
Takashi Nakamura
Takashi Nakamura
中科院分区:
--
文献类型:
--
作者:
H. Uehara;H. Susa;R. Nishi;M. Yamada;Takashi Nakamura

文献摘要

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讨论了退耦后宇宙中原始气体云的碎裂。通过比较崩塌和碎裂的时间尺度,得到了碎片的典型质量。我们表明,估计的质量给出了最小质量的一个片段,是从原始的气体云,基本上是确定的Mesirasekhar质量。
We discuss the fragmentation of primordial gas clouds in the universe after decoupling. Comparing the timescale of collapse with that of fragmentation, we obtain the typical mass of a fragment both numerically and analytically. We show that the estimated mass gives the minimum mass of a fragment that is formed from the primordial gas cloud and essentially determined by the Chandrasekhar mass.