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)