The Formation of Molecules in Contracting Interstellar Clouds
スポンサーリンク
概要
- 論文の詳細を見る
The abundances of atoms, molecules and ions in contracting interstellar clouds are investigated in the wide ranges of density (from 10 cm^<-3> to 10^7 cm^<-3>) and optical depth. Abundances of molecules are not in a steady state in optically thick stages because their reaction time scales are very long (10^<12.5>-10^<13.5> sec) compared with the contraction time scales. At some stage of contraction the abundances of neutral molecules become frozen, and the frozen abundances are considerably different from the steady-state abundances. The frozen abundances are mainly determined by the contraction time scale of the cloud. Especially, molecules containing carbon except for CO are less abundant for the cloud contracting more slowly.
- 理論物理学刊行会の論文
- 1976-10-25
著者
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鈴木 久男
北大理
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SUZUKI Hiroko
Department of Pediatrics, Graduate School of Medicine, Gifu University
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Nakagawa Yoshitsugu
Department of Cardiology, Graduate School of Comprehensive Human Sciences, University of Tsukuba
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Nakagawa Y
Department Of Earth And Planetary Sciences Faculty Of Science Kobe University
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Nakagawa Yoshitsugu
Department Of Physics Kyoto University
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MIKI Satoshi
Department of Physics, Kyoto University
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SATO Katsuhiko
Department of Physics, Kyoto University
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KIGUCHI Masayoshi
Department of Physics, Kyoto University
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Miki Satoshi
Department Of Bioresource Science Faculty Of Agriculture Kagawa University
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KIGUCHI Masayoshi
Research Institute for Science and Technology, Kinki University
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Suzuki Hiroko
Department Of Neuropsychiatry Nippon Medical School
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Sato Katsuhiko
Department Of Cardiovascular Medicine Hokkaido University School Of Medicine
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Kiguchi Masayoshi
Department Of Physics Kyoto University
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Miki Satoshi
Department Of Physics Kyoto University
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Miki Satoshi
Department Of Electronic Engineering Tokyo University Of Agriculture And Technology
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Suzuki Hiroko
Department Of Applied Physics Faculty Of Engineering Tohoku University:(present Address) Nippon Koga
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Suzuki Hiroko
Department Of Applied Chemistry Tokyo University Of Science
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KIGUCHI Masayoshi
Research Institute for Science and Technology Kinki University
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NAKAGAWA Yoshitsugu
Department of Physics, Kyoto University
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