H 2 formation on interstellar dust grains: the viewpoints of theory, experiments, models and observations
hal.structure.identifier | AMOR 2017 | |
hal.structure.identifier | Laboratoire d'Astrophysique de Bordeaux [Pessac] [LAB] | |
dc.contributor.author | WAKELAM, Valentine | |
hal.structure.identifier | Instituto de Ciencia de Materiales de Madrid [ICMM] | |
dc.contributor.author | BRON, Emeric | |
hal.structure.identifier | Delft University of Technology [TU Delft] | |
dc.contributor.author | CAZAUX, Stephanie | |
hal.structure.identifier | Laboratoire d'Etude du Rayonnement et de la Matière en Astrophysique [LERMA] | |
dc.contributor.author | DULIEU, Francois | |
hal.structure.identifier | Laboratoire d'Astrophysique de Marseille [LAM] | |
dc.contributor.author | GRY, Cecile | |
hal.structure.identifier | Institut d'Astrophysique de Paris [IAP] | |
dc.contributor.author | GUILLARD, Pierre | |
hal.structure.identifier | Institut d'astrophysique spatiale [IAS] | |
dc.contributor.author | HABART, Emilie | |
hal.structure.identifier | Interdisciplinary Nanoscience Center [iNANO] | |
dc.contributor.author | HORNEKAER, Liv | |
hal.structure.identifier | Laboratoire des Collisions Atomiques et Moléculaires | |
dc.contributor.author | MORISSET, Sabine | |
hal.structure.identifier | Göteborgs Universitet = University of Gothenburg [GU] | |
dc.contributor.author | NYMAN, Gunnar | |
hal.structure.identifier | Università degli studi di Catania = University of Catania [Unict] | |
dc.contributor.author | PIRRONELLO, Valerio | |
hal.structure.identifier | University College of London [London] [UCL] | |
dc.contributor.author | PRICE, Stephen | |
hal.structure.identifier | Laboratoire de Radioastronomie [LRA] | |
dc.contributor.author | VALDIVIA, Valeska | |
hal.structure.identifier | Syracuse University [Physics Department] | |
dc.contributor.author | VIDALI, Gianfranco | |
hal.structure.identifier | Institute of Low Temperature Science [Sapporo] | |
dc.contributor.author | WATANABE, Naoki | |
dc.date.issued | 2017 | |
dc.identifier.issn | 2405-6758 | |
dc.description.abstractEn | Molecular 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.iso | en | |
dc.publisher | Elsevier | |
dc.subject.en | Interstellar medium | |
dc.subject.en | Astrochemistry | |
dc.subject.en | Molecular hydrogen | |
dc.subject.en | Grain surface chemistry | |
dc.subject.en | Interstellar medium | |
dc.title.en | H 2 formation on interstellar dust grains: the viewpoints of theory, experiments, models and observations | |
dc.type | Article de revue | |
dc.identifier.doi | 10.1016/j.molap.2017.11.001 | |
dc.subject.hal | Planète et Univers [physics]/Astrophysique [astro-ph] | |
bordeaux.journal | Molecular Astrophysics | |
bordeaux.page | 1-36 | |
bordeaux.volume | 9 | |
bordeaux.peerReviewed | oui | |
hal.identifier | hal-01800298 | |
hal.version | 1 | |
hal.popular | non | |
hal.audience | Internationale | |
hal.origin.link | https://hal.archives-ouvertes.fr//hal-01800298v1 | |
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