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Shocks in Molecular Clouds
Published online by Cambridge University Press: 25 April 2016
Abstract
A one-day workshop discussed the properties of shocks in star-forming 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.
- Type
- Workshop Report
- Information
- Publications of the Astronomical Society of Australia , Volume 13 , Issue 3 , June 1996 , pp. 268 - 271
- Copyright
- Copyright © Astronomical Society of Australia 1996