Neutral radical-molecule reactions CO + OH on cold interstellar ices

Astronomy and Astrophysics – Astronomy

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Scientific paper

We investigated neutral radical-molecule reactions CO + OH without external energy inputs to investigate possible CO2 formation pathways inside dense molecular clouds, where UV field is relatively weak. OH radicals were produced by dissociating H2O in microwave-induced plasma and cooled down to 100 K before they were codeposited with CO on a cold Al surface at 10-40 K. Reaction products were monitored in-situ by FTIR spectroscopy. We observed the formation of CO2 in the reaction products. Furthermore, formation of trans- and cis-HOCO radicals were also identified. On this basis, we consider CO2 was formed by the following reactions on the cold Al surface:
CO + OH → cis-HOCO → trans-HOCO → CO_2 + H,
which have been proposed for the CO2 formation route in the gas phase. Our results suggest that the above reactions have little or no activation barrier. Conversion factor of CO to CO2 was up to 10 {%} under the present experimental conditions. In addition to CO2 and HOCO radicals, we found that carbonic acid, H2CO3, was formed probably by the following reactions:
HOCO + OH → H_2CO_3
H2CO3 has never been found in molecular clouds. However, if H2CO3 really exists in interstellar ices, it may act as an acid molecule to react with base molecules such as NH3, which results in the formation of NH4+, one of the possible candidates for the unidentified 6.8 μ m band observed toward various astronomical sources. Furthermore, we propose that H2CO3 itself could have a contribution to 6.8 μ m band.

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