An Optically Thin Inner Accretion Torus around a Weakly Magnetized Neutron Star
スポンサーリンク
概要
- 論文の詳細を見る
The optically thin inner region around an accreting weakly magnetized neutron star is examined using the a-model for viscous stress. We have found that a solution exists only for a limited range of C, an integration constant in the equation of conservation of angular momentum.
- 理論物理学刊行会の論文
- 1985-11-25
著者
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HOSHI Reiun
Department of Physics, Rikkyo University
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Hoshi Reiun
Department Of Physics Rikkyo University
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Hoshi Reiun
Department Of Physics Kyoto University
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HISHIKAWA Ikuko
Department of Physics, Rikkyo University
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Hishikawa Ikuko
Department Of Physics Rikkyo University
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HO-SHI Reiun
Department of Physics, Rikkyo University
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Hishikawa Ikuo
Department of Physics, Rikkyo University
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