Fast radiative shocks in dense media. I - General properties of the main shock

Details Fast radiative shocks in dense media. I - General properties of the main shock Fast radiative shocks in dense media. I - General properties of the main shock

Oct 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992aca....42..295p&link_type=abstract

Acta Astronomica (ISSN 0001-5237), vol. 42, no. 4, p. 295-309.

Astronomy and Astrophysics

Astrophysics

5

Active Galactic Nuclei, Cooling Flows (Astrophysics), Gas Dynamics, Shock Wave Propagation, Star Clusters, Ultraviolet Astronomy, Astronomical Models, Hydrodynamic Equations, Starburst Galaxies

Scientific paper

Hydrodynamical models of plane-parallel radiative shocks are presented for shock velocities not less than 1000 km/s. The post-shock regions and the shocks themselves are found to be highly nonstationary. Approximate light curves of the post-shock regions are obtained. The presence of a stochastic component is suggested in the variations of flow patterns, shock parameters, and emission rates, resulting mainly from the supersonic interactions between the post-main shock gas and the dense shell at the base of the post-shock region.

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