Hostname: page-component-586b7cd67f-r5fsc Total loading time: 0 Render date: 2024-12-05T02:32:38.229Z Has data issue: false hasContentIssue false
  • English
  • Français

Laboratory and Modeling Studies of Chemistry in Dense Molecular Clouds

Published online by Cambridge University Press:  14 August 2015

W.T. Huntress Jr. ,
S. S. Prasad  and
G. F. Mitchell
W.T. Huntress Jr.
Affiliation:
Jet Propulsion Laboratory, Pasadena, CA 91103.
S. S. Prasad
Affiliation:
Jet Propulsion Laboratory, Pasadena, CA 91103.
G. F. Mitchell
Affiliation:
Jet Propulsion Laboratory, Pasadena, CA 91103.

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

A 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.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 87: Interstellar Molecules , 1980 , pp. 331 - 336
Copyright
Copyright © Reidel 1980 

References

1. Prasad, S. S. and Huntress, W. T.: 1979, Astrophys. J. Suppl. Ser. in press.Google Scholar
2. Prasad, S. S. and Huntress, W. T.: 1979, Astrophys. J. in press.Google Scholar
3. Smith, D. and Adams, N. G.: 1978, Astrophys. J. (Letters) 220, p. L87.CrossRefGoogle Scholar
4. Huntress, W. T. and Mitchell, G. F.: 1979, Astrophys. J. 231, p. 456.Google Scholar
5. Mitchell, G. F., Huntress, W. T. and Prasad, S. S.: 1979, Astrophys. J. 233, p. 102.Google Scholar
6. McEwan, M.: private communication.Google Scholar