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Formation of Complex Molecules in Prestellar Cores: A Multilayer Approach
We present the results of chemical modeling of complex organic molecules (COMs) under conditions typical for prestellar cores. We utilize an advanced gas-grain astrochemical model with updated gas-phase chemistry, with a multilayer approach to ice-surface chemistry and an up-to-date treatment of reactive desorption based on recent experiments of Minissale et al. (2016). With the chemical model, radial profiles of molecules including COMs are calculated for the case of the prototypicaldoi:10.3847/1538-4357/aa72ec fatcat:jn55lywcc5cmtgffawuxlyo2iy