Response of Gas to an Ovally Deformed Gravitational Potential of a Disk Galaxy
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概要
- 論文の詳細を見る
The response of gas to an ovally deformed, rotating gravitational potential is investigated by following the time evolution of its motion using the Lin-Pringle quasi-particle technique. The results reveal that the gas responds to the presence of an oval distortion by forming a well-defined two-arm trailing spiral wave and elliptical rings rotating with angular speed of the oval distortion.
- 理論物理学刊行会の論文
- 1980-10-25
著者
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MATSUDA Takuya
Department of Aeronautical Engineering, Kyoto University
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ISAKA Hiromu
Department of Earth and Planetary Sciences, Kobe University
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Isaka Hiromu
Department Of Aeronautical Engineering Faculty Of Engineering Kyoto University
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Matsuda Takuya
Department Of Aeronautical Engineering Faculty Of Engineering Kyoto University
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ISAKA Hiromu
Department of Aeronautical Engineering, Faculty of Engineering, Kyoto University
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MATSUDA Takuya
Department of Aeronautical Engineering, Faculty of Engineering, Kyoto University
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