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Molecular shocks in star forming regions
Authors:P. W. J. L. Brand
Affiliation:(1) Institute for Astronomy, University of Edinburgh, Royal Observatory, EH9 3HJ Edinburgh, U.K.
Abstract:The role of excited molecular hydrogen as a powerful observational tool is examined in the context of shock phenomena in molecular clouds, particularly in star forming regions. Conclusions that may be drawn from line intensities and line profiles, and the properties of J and C shocks in a bow shock structure are discussed.
Keywords:Molecular hydrogen  shocks  outflows
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