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dc.contributor.authorWehmeyer, B.
dc.contributor.authorLópez, A. Yagüe
dc.contributor.authorCôté, B.
dc.contributor.authorPető, M.K.
dc.contributor.authorKobayashi, C.
dc.contributor.authorLugaro, M.
dc.date.accessioned2025-01-07T14:30:00Z
dc.date.available2025-01-07T14:30:00Z
dc.date.issued2024-06-07
dc.identifier.citationWehmeyer , B , López , A Y , Côté , B , Pető , M K , Kobayashi , C & Lugaro , M 2024 , ' Galactic chemical evolution with the short-lived isotopes 53Mn, 60Fe, 182Hf, and 244Pu ' , EPJ Web of Conferences , vol. 297 , 01016 , pp. 1-6 . https://doi.org/10.1051/epjconf/202429701016
dc.identifier.issn2101-6275
dc.identifier.otherRIS: urn:D34F83DED11761CDC7A5FD41487ACF1F
dc.identifier.otherRIS: 10.1051epjconf202429701016
dc.identifier.urihttp://hdl.handle.net/2299/28655
dc.description© 2024 The Authors, published by EDP Sciences. This is an open access article distributed under the Creative Commons Attribution License (CC BY), https://creativecommons.org/licenses/by/4.0/
dc.description.abstractWe run a three-dimensional Galactic chemical evolution (GCE) model to follow the propagation of 53Mn from supernovae of type Ia (SNIa), 60Fe from core-collapse supernovae (CCSNe), 182Hf from intermediate mass stars (IMSs), and 244Pu from neutron star mergers (NSMs) in the Galaxy. We compare the GCE of these short-lived radioactive isotopes (SLRs) to recent detections on the deep-sea floor. We find that although these SLRs originate from different sites, they often arrive conjointly on Earth.en
dc.format.extent6
dc.format.extent203742
dc.language.isoeng
dc.relation.ispartofEPJ Web of Conferences
dc.titleGalactic chemical evolution with the short-lived isotopes 53Mn, 60Fe, 182Hf, and 244Puen
dc.contributor.institutionCentre for Astrophysics Research (CAR)
dc.contributor.institutionSchool of Physics, Engineering & Computer Science
dc.contributor.institutionDepartment of Physics, Astronomy and Mathematics
dc.description.statusPeer reviewed
rioxxterms.versionofrecord10.1051/epjconf/202429701016
rioxxterms.typeOther
herts.preservation.rarelyaccessedtrue


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