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hal.structure.identifierInstitut des Sciences Moléculaires [ISM]
dc.contributor.authorHICKSON, Kevin M.,
hal.structure.identifierAMOR 2016
dc.contributor.authorWAKELAM, Valentine
hal.structure.identifierInstitut des Sciences Moléculaires [ISM]
dc.contributor.authorLOISON, Jean-Christophe,
dc.date.issued2016-03
dc.identifier.issn2405-6758
dc.description.abstractEnWe present an extensive review of gas phase reactions producing methylacetylene and propene showing that these relatively abundant unsaturated hydrocarbons cannot be synthesized through gas-phase reactions. We explain the formation of propene and methylacetylene through surface hydrogenation of C3 depleted onto interstellar ices, C3 being a very abundant species in the gas phase.
dc.language.isoen
dc.publisherElsevier
dc.subject.enPhysics - Chemical Physics
dc.subject.enAstrophysics - Astrophysics of Galaxies
dc.title.enMethylacetylene (CH3CCH) and propene (C3H6) formation in cold dense clouds: a case of dust grain chemistry
dc.typeArticle de revue
dc.identifier.doi10.1016/j.molap.2016.03.001
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Cosmologie et astrophysique extra-galactique [astro-ph.CO]
bordeaux.journalMolecular Astrophysics
bordeaux.page1-9
bordeaux.volume3
bordeaux.peerReviewedoui
hal.identifierhal-01291188
hal.version1
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-01291188v1
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