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Molecular Clouds near Supernova Remnants
Published online by Cambridge University Press: 14 August 2015
Abstract
A survey of 14 SNR's in the 4.8 GHz absorption line of H2CO shows that two of them, W28 and W44, possibly interact with molecular clouds. The interaction leads to acceleration of a part of the molecular cloud to a velocity of ∼5 km s-1 without a significant increase in the kinetic temperature or turbulence.
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- Research Article
- Information
- Symposium - International Astronomical Union , Volume 87: Interstellar Molecules , 1980 , pp. 473 - 478
- Copyright
- Copyright © Reidel 1980
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