Gravitationally driven instabilities in shock compressed gas layers

Details Gravitationally driven instabilities in shock compressed gas layers Gravitationally driven instabilities in shock compressed gas layers

Jan 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982a%26a...105..237w&link_type=abstract

Astronomy and Astrophysics, vol. 105, no. 2, Jan. 1982, p. 237-241. Research supported by the Deutsche Forschungsgemeinschaft.

Astronomy and Astrophysics

Astrophysics

14

Compressed Gas, Compressible Boundary Layer, Gravitational Effects, Shock Waves, Stellar Evolution, Perturbation Theory, Shock Fronts

Scientific paper

The paper examines the stability properties of shock compressed gas layers and the computational simplification of Elmegreen and Elmegreen (1978) and Welter and Schmid-Burgk (1981), which treats the layer as stationary and pressure bounded, rather than moving and shock bounded. The calculation assumes plane stratification for the unperturbed model. Results demonstrate that the use of a stationary, pressure bounded layer does not introduce significant error in calculating dispersion relations for gravitationally driven instabilities.

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