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dc.rights.license© 2020 The Author(s). Published by Oxford University Press on behalf of Royal Astronomical Society.-
dc.contributor.authorViti, S.-
dc.contributor.authorFontani, F.-
dc.contributor.authorJiménez Serra, I.-
dc.contributor.otherUnidad de Excelencia Científica María de Maeztu Centro de Astrobiología del Instituto Nacional de Técnica Aeroespacial y CSIC, MDM-2017-0737-
dc.date.accessioned2021-04-08T07:24:45Z-
dc.date.available2021-04-08T07:24:45Z-
dc.date.issued2020-07-18-
dc.identifier.citationMonthly Notices of the Royal Astronomical Society 497: 4333- 4345 (2020)es
dc.identifier.issn0035-8711-
dc.identifier.otherhttps://academic.oup.com/mnras/article-abstract/497/4/4333/5877251-
dc.identifier.urihttp://hdl.handle.net/20.500.12666/150-
dc.description.abstractIn the interstellar medium carbon exists in the form of two stable isotopes 12C and 13C and their ratio is a good indicator of nucleosynthesis in galaxies. However, chemical fractionation can potentially significantly alter this ratio and in fact observations of carbon fractionation within the same galaxy has been found to vary from species to species. In this paper, we theoretically investigate the carbon fractionation for selected abundant carbon-bearing species in order to determine the conditions that may lead to a spread of the 12C/13C ratio in external galaxies. We find that carbon fractionation is sensitive to almost all the physical conditions we investigated, it strongly varies with time for all species but CO, and shows pronounced differences across species. Finally, we discuss our theoretical results in the context of the few observations of the 12C/13C  in both local and higher redshift galaxies.es
dc.description.sponsorshipSV acknowledges support from the European Research Council (ERC) grant MOPPEX ERC-833460. SV and FF acknowledge the support of Science and Technology Facilities Council (STFC) (grant number ST/R000476/1) and the Center for Astrochemical Study at MPE for partially supporting this work. I.J.-S. has received partial support from the Spanish FEDER (project number ESP2017-86582-C4-1-R). We thank Prof Roueff for providing us the needed information to perform a benchmarking with her model, and the anonymous referee for their constructive comments which improved the manuscript. Also with funding from the Spanish government through the "María de Maeztu Unit of Excellence" accreditation (MDM-2017-0737)es
dc.language.isoenges
dc.publisherOxford Academics: Blackwell Publishinges
dc.relationinfo:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2013-2016/ESP2017-86582-C4-1-R/ES/CONTRIBUCION ESPAÑOLA A LAS MISIONES ESPACIALES CRIOGENICAS SPICA Y ATHENA, POST-OPERACIONES DE HERSCHEL Y EXPLOTACION CIENTIFICA MULTIFRECUENCIA/-
dc.rightsAttribution-NonCommercial-NoDerivatives 4.0 Internationales
dc.rights.urihttps://creativecommons.org/licenses/by-nc-nd/4.0/-
dc.subjectISM: abundanceses
dc.subjectISM: moleculeses
dc.subjectGalaxies: ISMes
dc.subjectMolecular Tracerses
dc.subjectGases
dc.subjectStar Formationes
dc.titleA chemical study of carbon fractionation in external galaxieses
dc.typeinfo:eu-repo/semantics/articlees
dc.contributor.orcid0000-0003-4493-8714-
dc.contributor.orcid0000-0003-0348-3418-
dc.contributor.orcid0000-0001-8504-8844-
dc.identifier.doi10.1093/mnras/staa2215-
dc.identifier.e-issn1365-2966-
dc.contributor.funderAgencia Estatal de Investigación (AEI)-
dc.contributor.funderEuropean Research Council (ERC)-
dc.contributor.funderScience and Technology Facilities Council (STFC)-
dc.description.peerreviewedPeer reviewes
dc.type.hasVersioninfo:eu-repo/semantics/publishedVersion-
dc.rights.accessRightsinfo:eu-repo/semantics/openAccess-
dc.type.coarhttp://purl.org/coar/resource_type/c_6501-
dc.relation.projectIDinfo:eu-repo/grantAgreement/EC/H2020/833460-
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