Dynamical Stability of Supermassive Gas-Star System
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概要
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The dynamical stability of supermassive gas-star system is investigated by the simplified analysis. The oscillation of a gas-star system around its gravitational equilibrium configuration in the fundamental mode is identical with that of two harmonic oscillators interacting with each other. The minimum amounts of stars reruired to stabilize the systems are determined in the post-Newtonian approximation.
- 理論物理学刊行会の論文
- 1975-11-25
著者
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Takarada Katsuo
Department Of Physics Kyoto Kogei Sen-i University : Nrc-nasa Resident Research Associate
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Takarada Katsuo
Department Of Physics Kyoto Technical University
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