NASA NTRS · 20210003738
Chemical Evolution of Protostellar Matter
Abstract
We reveiw the chemical processes that are improtant in the evolution form a molecular cloud core to a protostellar disk. These cover both gas phase and gas grain interactions. The current obsevational and theoretical state of this field are discussed.
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Whittet, D., Velusamy, T., Tielens, A., Blake, G., Bergin, E., van Dishoeck, E.. 1999-07-05. Chemical Evolution of Protostellar Matter. https://ntrs.nasa.gov/citations/20210003738
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