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The Formation of Interstellar Molecules via Radiative Association Reactions
Published online by Cambridge University Press: 14 August 2015
Abstract
The radiative association rate coefficients and their temperature dependences have been estimated for several likely interstellar ion-molecule reactions from laboratory collisional association rate data. They include the CH3+ + H2 and CH3+ + H2O reactions, which we suggest lead to CH4 and CH3OH respectively, and the critical association reaction C+ + H2.
- Type
- Research Article
- Information
- Symposium - International Astronomical Union , Volume 87: Interstellar Molecules , 1980 , pp. 323 - 324
- Copyright
- Copyright © Reidel 1980