Far-Infrared Rotational Transition Lines of the Interstellar Water Vapor
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概要
- 論文の詳細を見る
Far-infrared rotational transition lines of H_2) vapor are calculated to predict the line intensities under the condition of interstellar molecular clouds. Fractional populations for ortho- and para-H_2O molecules are obtained by solving a statistical equilibrium equation in which we employ recent data of H_2O-H_2 collisional excitation coefficients. Results are shown by presenting excitation temperature and optical depth for representative transition lines. Predicted intensities of several far-infrared lines are also demonstrated for a simplified cloud model.
- 理論物理学刊行会の論文
- 1983-01-25
著者
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SHIBAI Hiroshi
The Institute of Space and Astronautical Science
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MAIHARA Toshinori
Department of Physics, Kyoto University
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Shibai Hiroshi
Department Of Physics Nagoya University
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Maihara Toshinori
Department Of Physics Kyoto University
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Maihara Toshinori
Department of Astronomy, Kyoto University
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