Cooling of Pre-Galactic Gas Clouds by Hydrogen Molecule
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概要
- 論文の詳細を見る
According to the expanding hot universe model, neutralization of the cosmic plasma ceases at the stage of radiation temperature T_rsime4000°K. After then, a density contrast in the uniform medium grows into a contracting gas cloud with mass greater than 10^<5~6>Mxodoi. Hydrogen molecule is formed in the cloud after the stage of T_rsime300°K, and the thermal evolution is largely affected by the cooling through H_2, whose processes are studied quantitatively in this paper. The present paper is a preliminary one for a more interesting problem of galaxy formation.
- 理論物理学刊行会の論文
- 1969-08-25
著者
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Sato Humitaka
Department Of Physics Kyoto Univesity
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MATSUDA Takuya
Department of Aeronautical Engineering, Kyoto University
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TAKEDA Hidenori
Department of Physics, Kyoto University
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Sato Humitaka
Department Of Nuclear Science Kyoto University
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Matsuda Takuya
Department Of Aeronautical Engineering Kyoto University
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Takeda Hidenori
Department Of Aeronautical Engineering Kyoto University
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Matsuda Takuya
Department Of Aeronautical Engineering Faculty Of Engineering Kyoto University
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