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Gas-Dynamical Models of Star-forming Regions
Authors:AJ Lim
Institution:(1) University College London, UK
Abstract:This article describes some of the techniques used to include various micro-processes in numerical gas-dynamic simulations. These techniques are then used in simulations of photo-evaporating clumps, H2 level populations and time dependent shocks/jets. This revised version was published online in July 2006 with corrections to the Cover Date.
Keywords:Early universe  ISM: clouds  Herbig-Haro objects  jets and outflows  planetary nebulae
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