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hal.structure.identifierAMOR 2013
dc.contributor.authorWAKELAM, Valentine
dc.contributor.authorSMITH, I. W. M.
dc.contributor.authorLOISON, J. -C.
hal.structure.identifierLaboratoire Univers et Particules de Montpellier [LUPM]
dc.contributor.authorTALBI, D.
dc.contributor.authorKLIPPENSTEIN, S. J.
hal.structure.identifierInstitut des Sciences Moléculaires [ISM]
dc.contributor.authorBERGEAT, A.
dc.contributor.authorGEPPERT, W. D.
hal.structure.identifierInstitut des Sciences Moléculaires [ISM]
dc.contributor.authorHICKSON, K. M.
dc.date.created2013-10-16
dc.date.issued2013
dc.description39 pages, not published in refereed journal, datasheets are given in KIDA
dc.description.abstractEnPredictions of astrochemical models depend strongly on the reaction rate coefficients used in the simulations. We reviewed a number of key reactions for the chemistry of nitrogen-bearing species in the dense interstellar medium and proposed new reaction rate coefficients for those reactions. The details of the reviews are given in the form of a datasheet associated with each reaction. The new recommended rate coefficients are given with an uncertainty and a temperature range of validity and will be included in KIDA (http://kida.obs.u-bordeaux1.fr).
dc.language.isoen
dc.subject.enPhysical data and processes: astrochemistry -- Astronomical databases: miscellaneous -- ISM: abundances
dc.subject.enmolecules
dc.title.enReview of important reactions for the nitrogen chemistry in the interstellar medium
dc.typeAutre document
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Cosmologie et astrophysique extra-galactique [astro-ph.CO]
dc.subject.halPhysique [physics]/Astrophysique [astro-ph]/Cosmologie et astrophysique extra-galactique [astro-ph.CO]
dc.identifier.arxiv1310.4350
hal.identifierhal-00874485
hal.version1
hal.popularnon
hal.audienceNon spécifiée
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-00874485v1
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