A self-similar flow of self-gravitating gas behind a shock wave with increasing energy. I
From MaRDI portal
Publication:1837600
DOI10.1007/BF00648929zbMath0507.76113MaRDI QIDQ1837600
Publication date: 1982
Published in: Astrophysics and Space Science (Search for Journal in Brave)
self-similarmagnetogasdynamicshomothermalincreasing energynonuniform atmosphere at restpropelling contact surfaceRoche's model casespherical waveself-gravitatingenergy content of flow between shock front and contact surface time-dependent
Shock waves and blast waves in fluid mechanics (76L05) Gas dynamics (general theory) (76N15) Magnetohydrodynamics and electrohydrodynamics (76W05)
Related Items (3)
A self-similar flow of self-gravitating gas behind a spherical shock wave in magnetogasdynamics ⋮ Self-similar flows of a self-gravitating gas with increasing energy in uniform atmosphere ⋮ Self-similar solutions in the theory of flare-ups in novae. I
Cites Work
This page was built for publication: A self-similar flow of self-gravitating gas behind a shock wave with increasing energy. I