Shocks in molecular clouds

Details Shocks in molecular clouds Shocks in molecular clouds

Nov 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996pasa...13..268b&link_type=abstract

Publications Astronomical Society of Australia, vol. 13, no. 3, p. 268-271

Astronomy and Astrophysics

Astronomy

Interstellar Medium, Magnetohydrodynamics

Scientific paper

A one day workshop discussed the properties of shocks in starforming regions. It also reviewed other physical processes in star-forming molecular gas, and the progress in numerical modelling of such physics. Discussion concentrated on the complexity which instabilities in the gas flow bring to the analysis of shocks. The consensus was that progress will be made as the spatial/spectral resolution of shock measurements improves, and as numerical modelling of the nonlinear growth of instabilities becomes possible, potentially leading to statistical models of shock dynamics.

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