Self-Similar Homothermal Flow of Self-Gravitating Gas Behind Shock Wave
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概要
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Self-similar homothermal flows of self-gravitating gas behind the spherical shock wave propagating in a nonuniform atmosphere at rest are investigated. Using a similarity variable the solution corresponding to infinite star (p_1ccr^<-w>) has been constructed. Both numerical and particular analytical solutions are obtained. These solutions are compared with the corresponding solutions of the adiabatic flow.
- 社団法人日本物理学会の論文
- 1974-01-15