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Published 2000 | Version public
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Chemical Evolution of Protostellar Matter

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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.

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© 2000 University of Arizona Press.

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Eprint ID
34696
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CaltechAUTHORS:20121005-084938185

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Created
2012-10-10
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Updated
2020-03-09
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Division of Geological and Planetary Sciences (GPS)
Series Name
University of Arizona Space Science Series