Molecular synthesis in interstellar clouds - The radiative association reaction H + OH yields H2O + h/nu/

Details Molecular synthesis in interstellar clouds - The radiative association reaction H + OH yields H2O + h/nu/ Molecular synthesis in interstellar clouds - The radiative association reaction H + OH yields H2O + h/nu/

Jul 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980mnras.192....1f&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 192, July 1980, p. 1-10.

Other

7

Association Reactions, Hydrogen Clouds, Hydroxyl Radicals, Interstellar Chemistry, Interstellar Gas, Chemical Reactions, Free Radicals, Helium, Water

Scientific paper

On the evidence of some recent laboratory data on the association reaction H + OH + He yields H2O + He, and following previously proposed ion-neutral radiative association reaction schemes, it is suggested that the radiative association of H with OH can be a significant production mechanism for H2O in interstellar clouds, perhaps being a faster process for H2O production in some clouds than the ion-neutral reaction sequences. The H atom/radical radiative association process may be important in the production of other small molecules in interstellar clouds.

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