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• W3106131492 abstract "Aims.We have recently developed a microscopic Monte Carlo approach to study surface chemistry on interstellar grains and the morphology of ice mantles. The method is designed to eliminate the problems inherent in the rate-equation formalism to surface chemistry. Here we report the first use of this method in a chemical model of cold interstellar cloud cores that includes both gas-phase and surface chemistry. The surface chemical network consists of a small number of diffusive reactions that can produce molecular oxygen, water, carbon dioxide, formaldehyde, methanol and assorted radicals." @default.
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• W3106131492 date "2007-05-02" @default.
• W3106131492 modified "2023-10-16" @default.
• W3106131492 title "Gas-grain chemistry in cold interstellar cloud cores with a microscopic Monte Carlo approach to surface chemistry" @default.
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• W3106131492 doi "https://doi.org/10.1051/0004-6361:20077423" @default.
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