Protostar formation in the early universe

Naoki Yoshida, Kazuyuki Omukai, Lars Hernquist

研究成果: Article査読

278 被引用数 (Scopus)

抄録

The nature of the first generation of stars in the universe remains largely unknown. Observations imply the existence of massive primordial stars early in the history of the universe, and the standard theory for the growth of cosmic structure predicts that structures grow hierarchically through gravitational instability. We have developed an ab initio computer simulation of the formation of primordial stars that follows the relevant atomic and molecular processes in a primordial gas in an expanding universe. The results show that primeval density fluctuations left over from the Big Bang can drive the formation of a tiny protostar with a mass 1% that of the Sun. The protostar is a seed for the subsequent formation of a massive primordial star.

本文言語English
ページ(範囲)669-671
ページ数3
ジャーナルScience
321
5889
DOI
出版ステータスPublished - 2008 8 1
外部発表はい

ASJC Scopus subject areas

  • 一般

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