Modeling CO Photolysis Experiments and Disk Chemistry Using Line-by-Line Spectra for the Oxygen Isotopologues of CO

Details Modeling CO Photolysis Experiments and Disk Chemistry Using Line-by-Line Spectra for the Oxygen Isotopologues of CO Modeling CO Photolysis Experiments and Disk Chemistry Using Line-by-Line Spectra for the Oxygen Isotopologues of CO

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011lpi....42.2780l&link_type=abstract

42nd Lunar and Planetary Science Conference, held March 7–11, 2011 at The Woodlands, Texas. LPI Contribution No. 1608, p.2780

Physics

Scientific paper

Full line-by-line spectra are used to simulate CO photolysis experiments
and solar nebula chemistry. For the disk, a temperature-dependence of
the 'slope' is predicted which may be useful in ruling out some
self-shielding models.

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