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hal.structure.identifierAMOR 2017
hal.structure.identifierLaboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
dc.contributor.authorWAKELAM, Valentine
hal.structure.identifierInstituto de Ciencia de Materiales de Madrid [ICMM]
dc.contributor.authorBRON, Emeric
hal.structure.identifierDelft University of Technology [TU Delft]
dc.contributor.authorCAZAUX, Stephanie
hal.structure.identifierLaboratoire d'Etude du Rayonnement et de la Matière en Astrophysique [LERMA]
dc.contributor.authorDULIEU, Francois
hal.structure.identifierLaboratoire d'Astrophysique de Marseille [LAM]
dc.contributor.authorGRY, Cecile
hal.structure.identifierInstitut d'Astrophysique de Paris [IAP]
dc.contributor.authorGUILLARD, Pierre
hal.structure.identifierInstitut d'astrophysique spatiale [IAS]
dc.contributor.authorHABART, Emilie
hal.structure.identifierInterdisciplinary Nanoscience Center [iNANO]
dc.contributor.authorHORNEKAER, Liv
hal.structure.identifierLaboratoire des Collisions Atomiques et Moléculaires
dc.contributor.authorMORISSET, Sabine
hal.structure.identifierGöteborgs Universitet = University of Gothenburg [GU]
dc.contributor.authorNYMAN, Gunnar
hal.structure.identifierUniversità degli studi di Catania = University of Catania [Unict]
dc.contributor.authorPIRRONELLO, Valerio
hal.structure.identifierUniversity College of London [London] [UCL]
dc.contributor.authorPRICE, Stephen
hal.structure.identifierLaboratoire de Radioastronomie [LRA]
dc.contributor.authorVALDIVIA, Valeska
hal.structure.identifierSyracuse University [Physics Department]
dc.contributor.authorVIDALI, Gianfranco
hal.structure.identifierInstitute of Low Temperature Science [Sapporo]
dc.contributor.authorWATANABE, Naoki
dc.date.issued2017
dc.identifier.issn2405-6758
dc.description.abstractEnMolecular hydrogen is the most abundant molecule in the universe. It is the first one to form and survive photo-dissociation in tenuous environments. Its formation involves catalytic reactions on the surface of interstellar grains. The micro-physics of the formation process has been investigated intensively in the last 20 years, in parallel of new astrophysical observational and modeling progresses. In the perspectives of the probable revolution brought by the future satellite JWST, this article has been written to present what we think we know about the H 2 formation in a variety of interstellar environments.
dc.language.isoen
dc.publisherElsevier
dc.subject.enInterstellar medium
dc.subject.enAstrochemistry
dc.subject.enMolecular hydrogen
dc.subject.enGrain surface chemistry
dc.subject.enInterstellar medium
dc.title.enH 2 formation on interstellar dust grains: the viewpoints of theory, experiments, models and observations
dc.typeArticle de revue
dc.identifier.doi10.1016/j.molap.2017.11.001
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]
bordeaux.journalMolecular Astrophysics
bordeaux.page1-36
bordeaux.volume9
bordeaux.peerReviewedoui
hal.identifierhal-01800298
hal.version1
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-01800298v1
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