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Observational constraints on the origin of the elements – VI. Origin and evolution of neutron-capture elements as probed by the Gaia-ESO survey
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dc.contributor.author | Lian, Jianhui | |
dc.contributor.author | Storm, Nicholas | |
dc.contributor.author | Guiglion, Guillaume | |
dc.contributor.author | Serenelli, Aldo | |
dc.contributor.author | Cote, Benoit | |
dc.contributor.author | Karakas, Amanda I | |
dc.contributor.author | Boardman, Nicholas | |
dc.contributor.author | Bergemann, Maria | |
dc.date.accessioned | 2023-08-31T16:30:03Z | |
dc.date.available | 2023-08-31T16:30:03Z | |
dc.date.issued | 2023-10 | |
dc.identifier | 293402244 | |
dc.identifier | cb0b1bf0-cb37-4eaf-affd-dfd54201b566 | |
dc.identifier | 85169913671 | |
dc.identifier.citation | Lian , J , Storm , N , Guiglion , G , Serenelli , A , Cote , B , Karakas , A I , Boardman , N & Bergemann , M 2023 , ' Observational constraints on the origin of the elements – VI. Origin and evolution of neutron-capture elements as probed by the Gaia -ESO survey ' , Monthly Notices of the Royal Astronomical Society , vol. 525 , no. 1 , pp. 1329-1341 . https://doi.org/10.1093/mnras/stad2390 | en |
dc.identifier.issn | 0035-8711 | |
dc.identifier.other | Jisc: 1292970 | |
dc.identifier.uri | https://hdl.handle.net/10023/28279 | |
dc.description | AS acknowledges grants PID2019-108709GB-I00 from Ministry of Science and Innovation (MICINN, Spain), Spanish program Unidad de Excelencia María de Maeztu CEX2020-001058-M, 2021-SGR-1526 (Generalitat de Catalunya), and support from ChETEC-INFRA (EU project no. 101008324). MB and JL are supported through the Lise Meitner grant from the Max Planck Society. MB acknowledges support by the Collaborative Research centre SFB 881 (projects A5, A10), Heidelberg University, of the Deutsche Forschungsgemeinschaft (DFG, German Research Foundation). This project has received funding from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation programme (grant agreement no. 949173). | en |
dc.description.abstract | Most heavy elements beyond the iron peak are synthesized via neutron capture processes. The nature of the astrophysical sites of neutron capture processes is still very unclear. In this work, we explore the observational constraints of the chemical abundances of s-process and r-process elements on the sites of neutron-capture processes by applying Galactic chemical evolution (GCE) models to the data from Gaia-ESO large spectroscopic stellar survey. For the r-process, the [Eu/Fe]–[Fe/H] distribution suggests a short delay time of the site that produces Eu. Other independent observations (e.g. NS–NS binaries), however, suggest a significant fraction of long delayed (>1 Gyr) neutron star mergers (NSM). When assuming NSM as the only r-process sites, these two observational constraints are inconsistent at above 1σ level. Including short delayed r-process sites like magnetorotational supernova can resolve this inconsistency. For the s-process, we find a weak metallicity dependence of the [Ba/Y] ratio, which traces the s-process efficiency. Our GCE model with up-to-date yields of AGB stars qualitatively reproduces this metallicity dependence, but the model predicts a much higher [Ba/Y] ratio compared to the data. This mismatch suggests that the s-process efficiency of low-mass AGB stars in the current AGB nucleosynthesis models could be overestimated. | |
dc.format.extent | 13 | |
dc.format.extent | 1452378 | |
dc.language.iso | eng | |
dc.relation.ispartof | Monthly Notices of the Royal Astronomical Society | en |
dc.subject | Stars: abundances | en |
dc.subject | Stars: neutron | en |
dc.subject | Galaxy: evolution | en |
dc.subject | Galaxy: disc | en |
dc.subject | Stars: AGB and post-AGB | en |
dc.subject | QB Astronomy | en |
dc.subject | QC Physics | en |
dc.subject | DAS | en |
dc.subject.lcc | QB | en |
dc.subject.lcc | QC | en |
dc.title | Observational constraints on the origin of the elements – VI. Origin and evolution of neutron-capture elements as probed by the Gaia-ESO survey | en |
dc.type | Journal article | en |
dc.contributor.institution | University of St Andrews. School of Physics and Astronomy | en |
dc.identifier.doi | https://doi.org/10.1093/mnras/stad2390 | |
dc.description.status | Peer reviewed | en |
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