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THE 2014 KIDA NETWORK FOR INTERSTELLAR CHEMISTRY

hal.structure.identifierLaboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
dc.contributor.authorWAKELAM, V.
hal.structure.identifierInstitut des Sciences Moléculaires [ISM]
dc.contributor.authorLOISON, J.-C.
hal.structure.identifierUniversity of Virginia
dc.contributor.authorHERBST, Eric
hal.structure.identifierLaboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
dc.contributor.authorPAVONE, B.
hal.structure.identifierInstitut des Sciences Moléculaires [ISM]
dc.contributor.authorBERGEAT, Astrid
hal.structure.identifierInstitut des Sciences Moléculaires d'Orsay [ISMO]
dc.contributor.authorBÉROFF, K.
hal.structure.identifierInstitut de Physique Nucléaire d'Orsay [IPNO]
dc.contributor.authorCHABOT, M.
hal.structure.identifierInstitut de Planétologie et d'Astrophysique de Grenoble [IPAG ]
dc.contributor.authorFAURE, A.
hal.structure.identifierIstituto Nazionale di Astrofisica [INAF]
dc.contributor.authorGALLI, D.
hal.structure.identifierStockholm University
dc.contributor.authorGEPPERT, W.
hal.structure.identifierChemnitz University of Technology / Technische Universität Chemnitz
dc.contributor.authorGERLICH, D.
hal.structure.identifierLaboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
dc.contributor.authorGRATIER, P.
hal.structure.identifierLaboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
hal.structure.identifierInstitut des Sciences Moléculaires [ISM]
dc.contributor.authorHARADA, N.
hal.structure.identifierInstitut des Sciences Moléculaires [ISM]
dc.contributor.authorHICKSON, K.
hal.structure.identifierLaboratoire Interdisciplinaire Carnot de Bourgogne [ICB]
dc.contributor.authorHONVAULT, P.
hal.structure.identifierArgonne National Laboratory [Lemont] [ANL]
dc.contributor.authorKLIPPENSTEIN, S.
hal.structure.identifierInstitut de Physique de Rennes [IPR]
dc.contributor.authorLE PICARD, S.
hal.structure.identifierGöteborgs Universitet = University of Gothenburg [GU]
dc.contributor.authorNYMAN, G.
hal.structure.identifierLaboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
dc.contributor.authorRUAUD, M.
hal.structure.identifierUniversität zu Köln = University of Cologne
dc.contributor.authorSCHLEMMER, S.
hal.structure.identifierInstitut de Physique de Rennes [IPR]
dc.contributor.authorSIMS, I.
hal.structure.identifierLaboratoire Univers et Particules de Montpellier [LUPM]
dc.contributor.authorTALBI, D.
hal.structure.identifierUniversity College of London [London] [UCL]
dc.contributor.authorTENNYSON, J.
hal.structure.identifierUniversität Innsbruck [Innsbruck]
dc.contributor.authorWESTER, R.
dc.date.issued2015-03-25
dc.description.abstractEnChemical models used to study the chemical composition of the gas and the ices in the interstellar medium are based on a network of chemical reactions and associated rate coefficients. These reactions and rate coefficients are partially compiled from data in the literature, when available. We present in this paper kida.uva.2014, a new updated version of the kida.uva public gas-phase network first released in 2012. In addition to a description of the many specific updates, we illustrate changes in the predicted abundances of molecules for cold dense cloud conditions as compared with the results of the previous version of our network, kida.uva.2011.
dc.language.isoen
dc.publisherIOPscience
dc.subject.enastrochemistry
dc.subject.enastronomical databases: miscellaneous
dc.subject.enISM: abundances
dc.subject.enISM: molecules
dc.title.enTHE 2014 KIDA NETWORK FOR INTERSTELLAR CHEMISTRY
dc.typeArticle de revue
dc.identifier.doi10.1088/0067-0049/217/2/20
dc.subject.halPhysique [physics]
dc.identifier.arxiv1503.01594
bordeaux.journalThe Astrophysical Journal Supplement Series
bordeaux.page20
bordeaux.volume217
bordeaux.issue2
bordeaux.peerReviewedoui
hal.identifierhal-04159196
hal.version1
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-04159196v1
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