Rate of the reaction - OH + CO to CO2 + H at interstellar temperatures

Details Rate of the reaction - OH + CO to CO2 + H at interstellar temperatures Rate of the reaction - OH + CO to CO2 + H at interstellar temperatures

Oct 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988mnras.234.1059s&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 234, Oct. 15, 1988, p. 1059-1063.

Astronomy and Astrophysics

Astronomy

5

Carbon Dioxide, Carbon Monoxide, Hydroxyl Radicals, Interstellar Chemistry, Reaction Kinetics, Cryogenic Temperature, Gas Density, Hydrogen, Interstellar Gas, Stellar Envelopes

Scientific paper

The results of calculations of the rate constants for OH+CO→CO2+H are presented. They suggest that this reaction is at least an order-of-magnitude slower at temperatures below 70K than has previously been assumed. The only neutral-neutral reactions which are likely to be important in interstellar chemistry are those between two free radicals which can occur by successive bond-forming bond-breaking steps.

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