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hal.structure.identifierAMOR 2015
dc.contributor.authorWAKELAM, Valentine
dc.contributor.authorLOISON, J.-C.
dc.contributor.authorHICKSON, K. M.
hal.structure.identifierAMOR 2015
dc.contributor.authorRUAUD, M.
dc.date.issued2015
dc.identifier.issn1745-3925
dc.description.abstractEnThe ketenyl radical (HCCO) has recently been discovered in two cold dense clouds with a non-negligible abundance of a few 10-11 (compared to H2). Until now, no chemical network has been able to reproduce this observation. We propose here a chemical scheme that can reproduce HCCO abundances together with HCO, H2CCO and CH3CHO in the dark clouds Lupus-1A and L486. The main formation pathway for HCCO is the OH + CCH → HCCO + H reaction as suggested by Agúndez et al. but with a much larger rate coefficient than used in current models. Since this reaction has never been studied experimentally or theoretically, this larger value is based on a comparison with other similar systems.
dc.language.isoen
dc.publisherWiley-Blackwell
dc.subject.enastrochemistry
dc.subject.enISM: abundances
dc.subject.enISM: clouds
dc.subject.enISM: molecules
dc.title.enA proposed chemical scheme for HCCO formation in cold dense clouds
dc.typeArticle de revue
dc.identifier.doi10.1093/mnrasl/slv097
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Cosmologie et astrophysique extra-galactique [astro-ph.CO]
dc.identifier.arxiv1509.00336
bordeaux.journalMonthly Notice- Royal Astronomical Society -Letters-
bordeaux.pageL48-L52
bordeaux.volume453
bordeaux.issue1
bordeaux.peerReviewedoui
hal.identifierhal-01198427
hal.version1
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-01198427v1
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