Studying shocks in model astrophysical flows

Details Studying shocks in model astrophysical flows Studying shocks in model astrophysical flows

Feb 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apj...337l..89c&link_type=abstract

Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 337, Feb. 15, 1989, p. L89-L91.

Astronomy and Astrophysics

Astrophysics

11

Astronomical Models, Magnetohydrodynamic Flow, Shock Wave Propagation, Adiabatic Flow, Kepler Laws, Three Dimensional Flow, Transonic Flow

Scientific paper

We briefly discuss some properties of the shocks in the existing models for quasi-two-dimensional astrophysical flows. All of these models which allow the study of shocks analytically have some unphysical characteristics due to inherent assumptions made. We propose a hybrid model for a thin flow which has fewer unpleasant features and is suitable for the study of shocks.

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