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Observations of Shock Waves in Interstellar Clouds

Published online by Cambridge University Press:  14 August 2015

Steven Beckwith
Steven Beckwith*
Affiliation:
Department of Astronomy, Cornell University, Ithaca, N.Y., U.S.A.

Abstract

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Some techniques for observing shock waves in interstellar clouds are discussed. It is concluded that recent measurements of molecular hydrogen emission provide the best currently available technique for studying shocks. The results of measurements toward the Orion nebula are discussed, and a discussion and summary of the currently known H2 sources is given.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 87: Interstellar Molecules , 1980 , pp. 455 - 463
Copyright
Copyright © Reidel 1980 

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