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Laboratory and modeling studies of chemistry in dense molecular cloudsA chemical evolutionary model with a large number of species and a large chemical library is used to examine the principal chemical processes in interstellar clouds. Simple chemical equilibrium arguments show the potential for synthesis of very complex organic species by ion-molecule radiative association reactions.
Document ID
19810043315
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Huntress, W. T., Jr. (Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Prasad, S. S. (Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Mitchell, G. F. (California Institute of Technology, Jet Propulsion Laboratory, Pasadena Calif., United States)
Date Acquired
August 11, 2013
Publication Date
January 1, 1980
Subject Category
Astrophysics
Meeting Information
Meeting: Symposium on Interstellar molecules
Location: Mont Tremblant, Quebec
Country: Canada
Start Date: August 6, 1979
End Date: August 10, 1979
Accession Number
81A27719
Distribution Limits
Public
Copyright
Other

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