On the Mechanism of Stellar Explosion

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概要

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• In order to deal with dynamical phenomena of stars, gasdynamical equations and, especially, the shock relations are examined in relation to the stellar interior. The propagation of shock waves is then discussed, and especially the method developed by us is expounded. As an application, supernova explosion is treated in detail. The origin of planetary nebulae is also considered briefly.

• 理論物理学刊行会の論文

著者

• OHYAMA Noboru

  Department of Nuclear Science, Kyoto University

• Ohyama Noboru

  Department Of Nuclear Science Kyoto University

• Ono Yoro

  Institute Of Physics Hokkaido University

• Sakashita Shiro

  Institute Of Physics Hokkaido University

• ONO Yoro

  Institute of Physics, Hokkaido University

関連論文

• Stellar Synthesis of the α-Particle Nuclei Heavier than Ne^
• Propagation of Shock Waves in Inhomogeneous Medium. IV : Second Order Approximation
• Rapid Contraction of a Protostar to the Stage of Quasi-Hydrostatic Equilibrium. I : The Case of One Solar Mass without Radiation Flow
• On the Mechanism of Stellar Explosion

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