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CO2 formation in quiescent clouds: an experimental study of the CO + OH Pathway

Noble, J. A.; Dulieu, F.; Congiu, E. and Fraser, H. J. (2011). CO2 formation in quiescent clouds: an experimental study of the CO + OH Pathway. Astrophysical Journal, 735(2) p. 121.

DOI (Digital Object Identifier) Link: https://doi.org/10.1088/0004-637X/735/2/121
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Abstract

The formation of CO2 in quiescent regions of molecular clouds is not yet fully understood, despite CO2 having an abundance of around 10%–34% H2O. We present a study of the formation of CO2 via the nonenergetic route CO + OH on nonporous H2O and amorphous silicate surfaces. Our results are in the form of temperature-programmed desorption spectra of CO2 produced via two experimental routes: O2 + CO + H and O3 + CO + H. The maximum yield of CO2 is around 8% with respect to the starting quantity of CO, suggesting a barrier to CO + OH. The rate of reaction, based on modeling results, is 24 times slower than O2 + H. Our model suggests that competition between CO2 formation via CO + OH and other surface reactions of OH is a key factor in the low yields of CO2 obtained experimentally, with relative reaction rates of kCO+H « kCO+OH< k H2O2+H < kOH+H, kO2+H. Astrophysically, the presence of CO2 in low AV regions of molecular clouds could be explained by the reaction CO + OH occurring concurrently with the formation of H2O via the route OH + H.

Item Type: Journal Item
Copyright Holders: 2011 The American Astronomical Society
ISSN: 1538-4357
Keywords: astrochemistry; ISM - molecules; methods - laboratory
Academic Unit/School: Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
Faculty of Science, Technology, Engineering and Mathematics (STEM)
Item ID: 37238
Depositing User: Stephen Serjeant
Date Deposited: 16 Apr 2013 15:49
Last Modified: 02 May 2018 13:51
URI: http://oro.open.ac.uk/id/eprint/37238
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