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Observations of Shock Waves in Interstellar Clouds
Published online by Cambridge University Press: 14 August 2015
Abstract
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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