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Propagation of spherical shock waves in stars

https://doi.org/10.1017/s0022112056000275
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What this work says

Outgoing claims: the papers this work cites, builds on, or argues with.

inferredcites →https://doi.org/10.1002/cpa.3160060305openalex-snapshot
The propagation of weak spherical shocks in stars
inferredcites →https://doi.org/10.1073/pnas.37.8.495openalex-snapshot
Propagation of Spherical Shock Waves in Stellar Interiors
inferredcites →https://doi.org/10.1086/145892openalex-snapshot
The Propagation of Shock Waves in Self-Gravitating Gas Spheres.
inferredcites →https://doi.org/10.1098/rspa.1950.0049openalex-snapshot
The formation of a blast wave by a very intense explosion I. Theoretical discussion
inferredcites →https://doi.org/10.1098/rspa.1956.0069openalex-snapshot
The propagation and structure of shock waves of varying strength in a self-gravitating gas sphere
inferredcites →https://doi.org/10.1143/jpsj.8.662openalex-snapshot
On the Propagation and Structure of the Blast Wave, I

What points at this work

Incoming claims: where this work appears in other papers’ reference lists and arguments.

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Approximate analytical solution for the propagation of shock waves in self-gravitating perfect gas via power series method: isothermal flow
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Cylindrical shock wave propagation in a self-gravitating rotational axisymmetric perfect gas under the influence of azimuthal or axial magnetic field and monochromatic radiation with variable density
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Propagation of exponential shock wave in an axisymmetric rotating non-ideal dusty gas
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Group Invariance Method for Spherical Shock Wave in a Non-Ideal Gas under the Influence of Gravitational and Azimuthal Magnetic Fields
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Lie Group Theoretic Method for Magnetogasdynamic Shock Wave in a Rotational Axisymmetric Non-ideal Gas Under the Influence of Monochromatic Radiation
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Flow behind an exponential shock in a rotational axisymmetric mixture of non-ideal gas and small solid particles with heat conduction and radiation heat flux
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Cylindrical shock wave generated by a moving piston in a rotational axisymmetric non-ideal gas with conductive and radiative heat-fluxes in the presence of azimuthal magnetic field
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