Published 2000
| public
Book Section - Chapter
Chemical Evolution of Protostellar Matter
Chicago
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Abstract
We review the chemical processes that are important in the evolution from a molecular cloud core to a protostellar disk. These cover both gas-phase and gas-grain interactions. The current observational and theoretical status of this field are discussed.
Additional Information
© 2000 University of Arizona Press.Additional details
- Eprint ID
- 34696
- Resolver ID
- CaltechAUTHORS:20121005-084938185
- Created
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2012-10-10Created from EPrint's datestamp field
- Updated
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2020-03-09Created from EPrint's last_modified field
- Caltech groups
- Division of Geological and Planetary Sciences (GPS)
- Series Name
- University of Arizona Space Science Series