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dc.contributor.authorInostroza-Pino, Natalia
dc.contributor.authorMacLeod-Carey, Desmond
dc.contributor.authorHeyser, Cristopher
dc.contributor.authorMardones, Diego
dc.contributor.authorEspinoza, Carlos
dc.contributor.authorGe, Jixing
dc.date.accessioned2021-07-14T20:51:01Z
dc.date.available2021-07-14T20:51:01Z
dc.date.issued2021-06-01
dc.identifier10.1051/0004-6361/202140443
dc.identifier.issn00046361
dc.identifier.urihttps://hdl.handle.net/20.500.12728/9006
dc.description.abstractContext. Formaldehyde H2CO was the first organic polyatomic molecule discovered in the interstellar medium to have been detected in a variety of sources. However, pathways to synthesize this molecule under interstellar conditions have yet to be discussed. Aims. We carried out a systematic study to analyze the chemical processes that can explain the H2CO formation mechanism toward a decamer of methanol (CH3OH)10 as target material to mimic an ice mantle bombarded by an OH+ cation. Methods. We performed Born-Oppenheimer (ab initio) molecular dynamics simulations to obtain the formation mechanisms of complex organic molecules (COMs) such as formaldehyde H2CO and its HCOH isomer. Results. We found that CH2OH+ and CH2(OH)2 are the main precursors to form H2CO and HCOH. We discuss its formation mechanisms and the astrophysical implications in star-forming regions. These processes are likely relevant to the production of COMs.es_ES
dc.language.isoenes_ES
dc.publisherEDP Scienceses_ES
dc.subjectAstrochemistryes_ES
dc.subjectISM: moleculeses_ES
dc.subjectMolecular processeses_ES
dc.titleFormation of formaldehyde through methanol-ice-mantle (CH3OH)10bombardment by OH+cationes_ES
dc.typeArticlees_ES


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