Formation of Stars in Early Universe

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概要

• 論文の詳細を見る

• 本文データはCiNiiから複製したものである。Gravity which acts on optically thin gas makes the small sphericity in density fluctuation grow and causes fragmentation. As the first generation stars are formed from the density fluctuation at the decoupling epoch, it is important to study the thermal history of the density fluctuation taking account of the molecular process of hydrogen and deuteron.

• 近畿大学の論文
• 2004-02-28

著者

• Kiguchi Masayoshi

  RIST, Kinki University

• Kiguchi Masayoshi

  Rist Kinki University

関連論文

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• Implementation of Lagrange Scheme Code for Astrophysical Fluid Dynamics

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