Shock waves in a rotating, gravitating gaseous disk

Details Shock waves in a rotating, gravitating gaseous disk Shock waves in a rotating, gravitating gaseous disk

Aug 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979pazh....5..325f&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 5, July 1979, p. 325-331.) Soviet Astronomy Letters, vol. 5, July-Aug. 1979, p. 173-176

Astronomy and Astrophysics

Astronomy

4

Interstellar Gas, Rotating Disks, Shock Wave Propagation, Spiral Galaxies, Astronomical Models, Gravitational Fields, Shock Fronts, Viscosity

Scientific paper

A new type of shock wave which can exist only in a self-gravitating
system is analyzed. The treatment is illustrated by a simplified model
spiral galaxy - a rotating, gravitating gaseous disk. In such a disk the
oscillatory structure of the shock front will depend on the viscosity of
the gravitating gas.

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