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H2 in molecular shocks: observations from 2 to 12 microns
Authors:M J Richter  J R Graham  G S Wright  D M Kelly  J H Lacy
Institution:(1) University of California, Berkeley, USA;(2) Joint Astronomy Centre, USA;(3) The University of Texas at Austin, USA
Abstract:We present spectroscopy of the molecular shock in the supernova remnant IC 443. The H2 level populations in IC 443 are nearly identical to Orion Peak 1 (Brand et al. 1988; Parmar et al. 1994) and are consistent with a partially dissociative J-shock. The similarity with Orion suggests the shock processes which dominate the emission in both regions are essentially identical.
Keywords:Interstellar Molecules  Supernova Remnants  Infrared Spectroscopy
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