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• W2025192790 abstract "Context. Complex organic molecules are observed in a broad variety of astrophysical objects, but little is known about their formation mechanism. Laboratory simulations on interstellar ice analogues are therefore crucial for understanding the origin of these complex organic molecules. In this context, we focus on the thermal reactivity for the formation of the organic residue obtained after photolysis at 25 K of the interstellar ice analogue (H2O:CH3OH:NH3) warmed to 300 K." @default.
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• W2025192790 date "2013-03-01" @default.
• W2025192790 modified "2023-10-12" @default.
• W2025192790 title "Importance of thermal reactivity for hexamethylenetetramine formation from simulated interstellar ices" @default.
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• W2025192790 doi "https://doi.org/10.1051/0004-6361/201220870" @default.
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