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Chemical Evolution of Protostellar MatterWe 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.
Document ID
20210003738
Acquisition Source
Jet Propulsion Laboratory
Document Type
Other
External Source(s)
Authors
Whittet, D.
Velusamy, T.
Tielens, A.
Blake, G.
Bergin, E.
van Dishoeck, E.
Date Acquired
July 5, 1999
Publication Date
July 5, 1999
Publication Information
Publisher: UNKNOWN
Distribution Limits
Public
Copyright
Other
Technical Review
Keywords
protostellar
matter
solar
origins

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