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dc.contributor.authorRiedel, W.en
dc.contributor.authorSipilä, O.en
dc.contributor.authorRedaelli, E.en
dc.contributor.authorCaselli, P.en
dc.contributor.authorVasyunin, A. I.en
dc.contributor.authorDulieu, F.en
dc.contributor.authorWatanabe, N.en
dc.date.accessioned2024-04-05T16:38:15Z-
dc.date.available2024-04-05T16:38:15Z-
dc.date.issued2023-
dc.identifier.citationRiedel, W, Sipilä, O, Redaelli, E, Caselli, P, Vasyunin, A, Dulieu, F & Watanabe, N 2023, 'Modelling deuterated isotopologues of methanol towards the pre-stellar core L1544', Astronomy and Astrophysics, Том. 680, A87. https://doi.org/10.1051/0004-6361/202245367harvard_pure
dc.identifier.citationRiedel, W., Sipilä, O., Redaelli, E., Caselli, P., Vasyunin, A., Dulieu, F., & Watanabe, N. (2023). Modelling deuterated isotopologues of methanol towards the pre-stellar core L1544. Astronomy and Astrophysics, 680, [A87]. https://doi.org/10.1051/0004-6361/202245367apa_pure
dc.identifier.issn0004-6361-
dc.identifier.otherFinal2
dc.identifier.otherAll Open Access, Hybrid Gold, Green3
dc.identifier.otherhttps://www.scopus.com/inward/record.uri?eid=2-s2.0-85180548714&doi=10.1051%2f0004-6361%2f202245367&partnerID=40&md5=30c74ee04fdc06ba1788870338356c931
dc.identifier.otherhttps://doi.org/10.1051/0004-6361/202245367pdf
dc.identifier.urihttp://elar.urfu.ru/handle/10995/131075-
dc.description.abstractContext. In the extremely cold and dark environments of pre-stellar cores, methanol is formed on the surface of interstellar dust grains and released into the gas phase via non-thermal desorption mechanisms. Gaseous methanol constitutes the starting point for the formation of many massive complex organic molecules and is therefore of utmost importance for the build-up of chemical complexity. Aims. We aim to improve upon a previous model for the prediction of column densities and deuterium fractions of non-deuterated and singly deuterated methanol. Thereby, we try to identify crucial chemical and physical parameters for which the study of deuteration could provide valuable additional constraints. Methods. We employed a gas-grain chemical code to devise a model that is in agreement with the observed column density and deuterium fraction profiles of the innermost region of the pre-stellar core L1544. For that purpose, we developed a new treatment of reactive desorption, deriving an individual reactive desorption efficiency for every product species in a chemical reaction that depends on the reaction enthalpy and type of the underlying surface. Furthermore, we explored several options to promote the diffusion of hydrogen and deuterium atoms over the surface of interstellar dust grains in order to increase methanol formation. Results. Our fiducial model employs diffusion via the quantum tunnelling of hydrogen and deuterium atoms, resulting in CH3OH and CH2DOH column densities that are approximately an order of magnitude lower than the observed values, which is an improvement over the results of the previous model by a factor of 10. The N(CH2DOH)/N(CH3OH) ratio is reproduced within a factor of 1.2 for the centre and 1.8 for the position of the methanol peak. Given the large uncertainties that chemical models typically have, we consider our predictions to be in agreement with the observations. In general, we conclude that a diffusion process with a high diffusion rate needs to be employed to obtain methanol column densities that are in accordance with the observed values. Also, we find that the introduction of abstraction reactions into the methanol formation scheme suppresses deuteration when used in combination with a high diffusion rate. © The Authors 2023.en
dc.description.sponsorshipMinistry of Science and Higher Education of the Russian Federation: FEUZ-2020-0038en
dc.description.sponsorshipThe work by A.V. is supported by the Russian Ministry of Science and Higher Education via the Project FEUZ-2020-0038.en
dc.format.mimetypeapplication/pdfen
dc.language.isoenen
dc.publisherEDP Sciencesen
dc.rightsinfo:eu-repo/semantics/openAccessen
dc.rightscc-byother
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/unpaywall
dc.sourceAstronomy & Astrophysics2
dc.sourceAstronomy and Astrophysicsen
dc.subjectASTROCHEMISTRYen
dc.subjectISM: ABUNDANCESen
dc.subjectISM: CLOUDSen
dc.subjectISM: INDIVIDUAL OBJECTS: L1544en
dc.subjectISM: MOLECULESen
dc.subjectSTARS: FORMATIONen
dc.subjectDESORPTIONen
dc.subjectDIFFUSIONen
dc.subjectDUSTen
dc.subjectHYDROGENen
dc.subjectMETHANOLen
dc.subjectMOLECULESen
dc.subjectSTARSen
dc.subjectSURFACE REACTIONSen
dc.subjectASTROCHEMISTRYen
dc.subjectCOLUMN DENSITYen
dc.subjectINTERSTELLAR DUSTen
dc.subjectISM : CLOUDSen
dc.subjectISM: ABUNDANCEen
dc.subjectISM: INDIVIDUAL OBJECT: L1544en
dc.subjectISM: INDIVIDUAL OBJECTSen
dc.subjectISM:MOLECULESen
dc.subjectPRESTELLAR CORESen
dc.subjectSTARS FORMATIONen
dc.subjectDEUTERIUMen
dc.titleModelling deuterated isotopologues of methanol towards the pre-stellar core L1544en
dc.typeArticleen
dc.typeinfo:eu-repo/semantics/articleen
dc.type|info:eu-repo/semantics/publishedVersionen
dc.identifier.doi10.1051/0004-6361/202245367-
dc.identifier.scopus85180548714-
local.contributor.employeeRiedel, W., Max-Planck-Institut für Extraterrestrische Physik, Gießenbachstraße 1, Garching bei München, 85748, Germanyen
local.contributor.employeeSipilä, O., Max-Planck-Institut für Extraterrestrische Physik, Gießenbachstraße 1, Garching bei München, 85748, Germanyen
local.contributor.employeeRedaelli, E., Max-Planck-Institut für Extraterrestrische Physik, Gießenbachstraße 1, Garching bei München, 85748, Germanyen
local.contributor.employeeCaselli, P., Max-Planck-Institut für Extraterrestrische Physik, Gießenbachstraße 1, Garching bei München, 85748, Germanyen
local.contributor.employeeVasyunin, A.I., Ural Federal University, 19 Mira street, Yekaterinburg, 620002, Russian Federationen
local.contributor.employeeDulieu, F., CY Cergy Paris Université, Sorbonne Université, Observatoire de Paris, PSL University, CNRS, LERMA, Cergy, 95000, Franceen
local.contributor.employeeWatanabe, N., Institute of Low Temperature Science, Hokkaido University, Hokkaido, Sapporo, 060-0819, Japanen
local.volume680-
dc.identifier.wos001125494400018-
local.contributor.departmentMax-Planck-Institut für Extraterrestrische Physik, Gießenbachstraße 1, Garching bei München, 85748, Germanyen
local.contributor.departmentUral Federal University, 19 Mira street, Yekaterinburg, 620002, Russian Federationen
local.contributor.departmentCY Cergy Paris Université, Sorbonne Université, Observatoire de Paris, PSL University, CNRS, LERMA, Cergy, 95000, Franceen
local.contributor.departmentInstitute of Low Temperature Science, Hokkaido University, Hokkaido, Sapporo, 060-0819, Japanen
local.identifier.pure50621099-
local.description.orderA87-
local.identifier.eid2-s2.0-85180548714-
local.identifier.wosWOS:001125494400018-
Располагается в коллекциях:Научные публикации ученых УрФУ, проиндексированные в SCOPUS и WoS CC

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