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Chemical Evolution of Protostellar MatterWe 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 state of this field are discussed.
Document ID
20000057044
Acquisition Source
Jet Propulsion Laboratory
Document Type
Other
Authors
Langer, William D. (Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA United States)
vanDishoeck, Ewine F. (Leiden Observatory Leiden Netherlands)
Bergin, Edwin A. (Smithsonian Astrophysical Observatory Cambridge, MA United States)
Blake, Geoffrey A. (California Inst. of Tech. CA United States)
Tielens, Alexander G. G. M. (Kapteyn Astronomical Inst. Netherlands)
Velusamy, Thangasamy (Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA United States)
Whittet, Douglas C. B. (Rensselaer Polytechnic Inst. Troy, NY United States)
Date Acquired
September 7, 2013
Publication Date
January 1, 2000
Subject Category
Astrophysics
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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