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• W2029880025 abstract "Context. Understanding the gas abundance distribution is essential when tracing star formation using molecular line observations. Variations in density and temperature conditions can cause gas to freeze-out onto dust grains, and this needs to be taken into account when modeling a collapsing molecular cloud." @default.
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• W2029880025 date "2008-08-08" @default.
• W2029880025 modified "2023-09-27" @default.
• W2029880025 title "Time-dependent CO depletion during the formation of protoplanetary disks" @default.
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• W2029880025 doi "https://doi.org/10.1051/0004-6361:200810035" @default.
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