The dynamic and gravitational instabilities of spherical shocks

This paper examines the stability of a thin, spherical shock against dynamic and gravitational perturbations when the wavelength of the perturbation is large compared to the thickness of the dense shell. For dynamic perturbations, it is found that a spherical isothermal shock, driven by a hot gas, i...

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Bibliographic Details
Published inThe Astrophysical journal Vol. 274; no. 1; pp. 152 - 167
Main Author Vishniac, E. T.
Format Journal Article
LanguageEnglish
Published Chicago, IL University of Chicago Press 01.11.1983
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