Hydrogen Molecule Formation in the Collapsing Phase of Initial Cosmological Perturbation

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概要

• 論文の詳細を見る

• 本文データの一部は、CiNiiから複製したものである。Using second order Zel'dvich approximation, the thermal history and the hydrogen molecule abundance in growing cores of first generation objects is studied. The applicability of Zel'dvich approximation is checked by comparing two different methods. The result will play the bases for future observations.

• 近畿大学の論文
• 2003-02-28

著者

• Kiguchi Masayoshi

  近畿大学理工学総合研究所

関連論文

• Primordial Solar Nebula Embedded in Corona
• Morphology of Distant Galaxies
• Hydrogen Molecule Formation in the Collapsing Phase of Initial Cosmological Perturbation
• Note on Wind from T Tauri Stars〔和文〕
• An Attempt on the High Resolution Calculation by the Nested Grid Method
• Formation of first generation stars

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