A Steady State Model of X-Ray Emitting Coronae around Accreting Non-Magnetic White Dwarfs in Cataclysmic Variables
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概要
- 論文の詳細を見る
- Astronomical Society of Japanの論文
- 1999-02-25
著者
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尾崎 洋二
日本天文学会
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MAHASENA Putra
Department of Astronomy, School of Science, The University of Tokyo
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OSAKI Yoji
Department of Astronomy, School of Science, The University of Tokyo
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Mahasena P
Inst. Space And Astronautical Sci. Kanagawa
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Osaki Yoji
Department Of Astronomy School Of Science The University Of Tokyo
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