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The Nature of Shocks in Molecular Clouds

Published online by Cambridge University Press:  12 April 2016

Peter W. J. L. Brand*
Affiliation:
Department of Astronomy, University of EdinburghRoyal Observatory Edinburgh EH9 3HJ, U.K.

Abstract

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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
Copyright
Copyright © Springer-Verlag 1989

References

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