van Dishoeck, Ewine F. (1992) The Chemistry of Translucent and High-Latitude Molecular Clouds. In: Chemistry and Spectroscopy of Interstellar Molecules. University of Tokyo Press , Tokyo, pp. 69-74. ISBN 9784130682053 http://resolver.caltech.edu/CaltechAUTHORS:20121008-095502287
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Abstract
The chemical and physical structure of translucent and high-latitude interstellar clouds is reviewed with reference to recent observational results. Current steady-state gas-phase models can explain the measured abundances of simple molecules such as CH, C_2 and OH, but fail to reproduce the observed column densities of more complex molecules such as H_2CO and C_3H_2. The importance of grain-surface chemistry and shock-heated chemistry in these clouds is discussed.
| Item Type: | Book Section |
|---|---|
| Record Number: | CaltechAUTHORS:20121008-095502287 |
| Persistent URL: | http://resolver.caltech.edu/CaltechAUTHORS:20121008-095502287 |
| Usage Policy: | No commercial reproduction, distribution, display or performance rights in this work are provided. |
| ID Code: | 34746 |
| Collection: | CaltechAUTHORS |
| Deposited By: | Tony Diaz |
| Deposited On: | 10 Oct 2012 17:24 |
| Last Modified: | 10 Oct 2012 17:24 |
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