Theory of the gradient instabilities of the gaseous galactic disk and rotating shallow water

Details Theory of the gradient instabilities of the gaseous galactic disk and rotating shallow water Theory of the gradient instabilities of the gaseous galactic disk and rotating shallow water

Oct 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990zhetf..98.1121f&link_type=abstract

Zhurnal Eksperimental'noi i Teoreticheskoi Fiziki (ISSN 0044-4510), vol. 98, Oct. 1990, p. 1121-1137. In Russian.

Computer Science

Sound

10

Galactic Rotation, Galactic Structure, Rotating Fluids, Spiral Galaxies, Astronomical Models, Rarefied Gas Dynamics, Viscous Fluids

Scientific paper

A stability theory is presented for a rotating gaseous disk and a rotating shallow water layer in the case of discontinuities in the rotation and sound velocities. Various instabilities of subsonic and supersonic flows are examined. The equivalence of a system of dynamic linearized equations of the gaseous galactic disk and of rotating shallow water is demonstrated using simulations on the Spiral system.

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