Self-similar solutions in the theory of flare-ups in novae. I

DOI10.1007/BF00661159zbMath0578.76051MaRDI QIDQ1066753

J. B. Singh, P. R. Vishwakarma

Publication date: 1983

Published in: Astrophysics and Space Science (Search for Journal in Brave)

zbMATH Keywords

similarity solutionssupernovaeself-gravitating gasnon-uniform atmospherecentral stellar explosionsflare-ups in novaehomothermal flowsrear flow fieldspherical shock-wave

Mathematics Subject Classification ID

Shock waves and blast waves in fluid mechanics (76L05) Galactic and stellar dynamics (85A05) Stability and instability of geophysical and astrophysical flows (76E20)

Related Items (6)

Propagation of an exponential shock wave in a rotational axisymmetric isothermal or adiabatic flow of a self-gravitating non-ideal gas under the influence of axial or azimuthal magnetic field ⋮ Similarity solutions for strong shock waves in magnetogasdynamics under a gravitational field ⋮ Similarity solutions for cylindrical shock wave in self‐gravitating non‐ideal gas with axial magnetic field: Isothermal flow ⋮ Approximate analytical solution for ionizing cylindrical magnetogasdynamic shock wave in rotational axisymmetric self-gravitating perfect gas: isothermal flow ⋮ Magnetogasdynamic exponential shock wave in a self-gravitating, rotational axisymmetric non-ideal gas under the influence of heat-conduction and radiation heat-flux ⋮ Self-similar solutions in the theory of flare-ups in novae. II

Cites Work

• Unnamed Item
• Self-similar solutions in the theory of flare-ups in novae. II
• A self-similar flow of self-gravitating gas behind a shock wave with increasing energy. I

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