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hal.structure.identifierAMOR 2017
dc.contributor.authorMAJUMDAR, Liton
hal.structure.identifierAMOR 2017
dc.contributor.authorGRATIER, P.
hal.structure.identifierAMOR 2017
dc.contributor.authorRUAUD, M.
hal.structure.identifierAMOR 2017
dc.contributor.authorWAKELAM, Valentine
hal.structure.identifierCentre d'étude spatiale des rayonnements [CESR]
hal.structure.identifierCentre d'étude spatiale des rayonnements [CESR]
dc.contributor.authorVASTEL, C.
dc.contributor.authorSIPILÄ, O.
hal.structure.identifierECLIPSE 2017
dc.contributor.authorHERSANT, F.
hal.structure.identifierAMOR 2017
dc.contributor.authorDUTREY, Anne
hal.structure.identifierAMOR 2017
dc.contributor.authorGUILLOTEAU, S.
dc.date.issued2017
dc.identifier.issn0035-8711
dc.description.abstractEnDeuterated species are unique and powerful tools in astronomy since they can probe the physical conditions, chemistry, and ionization level of various astrophysical media. Recent observations of several deuterated species along with some of their spin isomeric forms have rekindled the interest for more accurate studies on deuterium fractionation. This paper presents the first publicly available chemical network of multiply deuterated species along with spin chemistry implemented on the latest state-of-the-art gas-grain chemical code `NAUTILUS'. D/H ratios for all deuterated species observed at different positions of TMC-1 are compared with the results of our model, which considers multiply deuterated species along with the spin chemistry of light hydrogen bearing species H2, H2+, H3+ and their isotopologues. We also show the differences in the modeled abundances of non-deuterated species after the inclusion of deuteration and spin chemistry in the model. Finally, we present a list of potentially observable deuterated species in TMC-1 awaiting detection.
dc.language.isoen
dc.publisherOxford University Press (OUP): Policy P - Oxford Open Option A
dc.subject.enAstrophysics - Astrophysics of Galaxies
dc.title.enChemistry of TMC-1 with multiply deuterated species and spin chemistry of H2, H2+, H3+ and their isotopologues
dc.typeArticle de revue
dc.identifier.doi10.1093/mnras/stw3360
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Cosmologie et astrophysique extra-galactique [astro-ph.CO]
dc.identifier.arxiv1612.07845
bordeaux.journalMonthly Notices of the Royal Astronomical Society
bordeaux.page4470-4479
bordeaux.volume466
bordeaux.peerReviewedoui
hal.identifierhal-01434936
hal.version1
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-01434936v1
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