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The Nature of Shocks in Molecular Clouds
Published online by Cambridge University Press: 12 April 2016
Abstract
Evidence is presented to suggest that the shocked molecular hydrogen emission in the brightest part of the Orion outflow is produced in a J-shock and not a C-shock; that this is true throughout the entire flow; that it may be true in many outflow sources; and that this exacerbates problems with current explanations of the very wide velocity profiles observed in molecular hydrogen emission.
- Type
- I. Molecular Clouds, Star Formation And HII Regions
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- Copyright © Springer-Verlag 1989