期刊
ASTROPHYSICAL JOURNAL
卷 942, 期 1, 页码 -出版社
IOP Publishing Ltd
DOI: 10.3847/1538-4357/ac97e3
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The study explores the formation of complex organic molecules in interstellar ice analogs composed of methanol and carbon dioxide using simulated secondary electrons generated in the track of galactic cosmic rays. Detecting the reaction products as they sublime, the researchers identify carbonic acid monomethyl ester (CH3OCOOH) and glycolic acid (HOCH2COOH) in the processed ices. The abundance of these molecules in analog interstellar ices and the low irradiation dose needed for their formation makes them excellent candidates for interstellar detection, unlike tautomers dihydroxyacetaldehyde ((OH)(2)CCHO) and enol ethenetriol (HOCHC(OH)(2)), which were not found to form under the applied conditions.
The formation of complex organic molecules by simulated secondary electrons generated in the track of galactic cosmic rays was investigated in interstellar ice analogs composed of methanol and carbon dioxide. The processed ices were subjected to temperature-programmed desorption to mimic the transition of a cold molecular cloud to a warmer star-forming region. Reaction products were detected as they sublime using photoionization reflectron time-of-flight mass spectrometry. By employing isotopic labeling, tunable photoionization and computed adiabatic ionization energies isomers of C2H4O3 were investigated. Product molecules carbonic acid monomethyl ester (CH3OCOOH) and glycolic acid (HOCH2COOH) were identified. The abundance of the reactants detected in analog interstellar ices and the low irradiation dose necessary to form these products indicates that these molecules are exemplary candidates for interstellar detection. Molecules sharing a tautomeric relationship with glycolic acid, dihydroxyacetaldehyde ((OH)(2)CCHO), and the enol ethenetriol (HOCHC(OH)(2)), were not found to form despite ices being subjected to conditions that have successfully produced tautomerization in other ice analog systems.
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