GRAIN SURFACE FORMATION OF METHYL FORMATE IN THE WARM-UP PHASE OF HOT MOLECULAR CORES
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Abstract
Until recently, the methyl formate detected in hot molecular cores in interstellar clouds was thought to originate from gas phase chemistry. However, recent theoretical work (Horn et al. 2004) has shown that there is a large potential barrier to the reaction between protonated methanol and formaldehyde which was thought to form protonated methyl formate. In addition to this, experimental results suggest that the recombination reaction of this precursor molecule with electrons should have only a very weak channel producing methyl formate. Other possible gas phase mechanisms were suggested by Horn et al. (2004), however, none were successful at the typical hot core temperature of 100 K. Most hot core chemical models consider only the hot period itself, or use a step-change in temperature. Here we consider a more detailed model of hot core evolution, invoking a warm-up phase of order 10
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Author Institution: Department of Physics, Ohio State University, 191 W. Woodruff Ave, Columbus, OH 43210