The Effect of Pressure Gradient Force on an Accretion Disk Surrounding a Black-Hole
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概要
- 論文の詳細を見る
A stationary thin-orbiting accretion disk surrounding a black-hole has been studied taking the pressure gradient force into account. We have found that under the condition appropriate for a binary X-ray source, with usual assumptions about viscous stress, the disk is largely modified when the pressure gradient force is taken into account. Therefore, current thin-disk models to account for observations of Cyg X-1 are self-inconsistent, since the pressure gradient force is neglected in those accretion disk models.
- 理論物理学刊行会の論文
- 1977-12-25
著者
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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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Shibazaki Noriaki
Department Of Physics Rikkyo University
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HO-SHI Reiun
Department of Physics, Rikkyo University
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