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dc.contributor.authorDonnan, Callum T.
dc.contributor.authorTojeiro, Rita
dc.contributor.authorKraljic, Katarina
dc.date.accessioned2022-09-13T23:41:15Z
dc.date.available2022-09-13T23:41:15Z
dc.date.issued2022-03-14
dc.identifier.citationDonnan , C T , Tojeiro , R & Kraljic , K 2022 , ' The role of the cosmic web in the scatter of the galaxy stellar mass - gas metallicity relation ' , Nature Astronomy , vol. Advance Article . https://doi.org/10.1038/s41550-022-01619-wen
dc.identifier.issn2397-3366
dc.identifier.otherPURE: 278087617
dc.identifier.otherPURE UUID: 86923624-709a-41b7-ac13-62b03e8f4bbf
dc.identifier.otherArXiv: http://arxiv.org/abs/2201.08757v1
dc.identifier.otherScopus: 85126239890
dc.identifier.otherWOS: 000768664000002
dc.identifier.urihttp://hdl.handle.net/10023/26005
dc.descriptionFunding for the Sloan Digital Sky Survey IV has been provided by the Alfred P. Sloan Foundation, the U.S. Department of Energy Office of Science, and the Participating Institutions.en
dc.description.abstractThe large-scale structure of the Universe can be understood in terms of features such as filaments, nodes and walls, which we collectively term the cosmic web. Galaxies evolve within the cosmic web, naturally raising the question of its impact on that process. There are two main mechanisms by which the cosmic web can influence galaxies: one is by modulating the growth of haloes, and the other is by regulating the gas ecosystem around galaxies. Disentangling the two is difficult, but key to deriving a holistic picture of galaxy formation and observational constraints on the growth of haloes. Here we report a detection of the effect of the cosmic web on the galaxy stellar mass–gas-phase metallicity relation of low-redshift star-forming galaxies using data from the Sloan Digital Sky Survey. The proximity of a galaxy to a node, independently of stellar mass and overdensity, influences its gas-phase metallicity, with galaxies closer to nodes displaying higher chemical enrichment than those farther away. We find a similar, but notably weaker, effect with respect to filaments. We find qualitative agreement in the cosmological hydrodynamical simulation IllustrisTNG (TNG300). Using IllustrisTNG, our results can be explained by both halo assembly bias and gas supply combining in nodes in a way that markedly modulates the metallicity of the gas, contributing to the scatter of this fundamental relation in galaxy evolution.
dc.language.isoeng
dc.relation.ispartofNature Astronomyen
dc.rightsCopyright © 2022, The Author(s), under exclusive licence to Springer Nature Limited. This work has been made available online in accordance with publisher policies or with permission. Permission for further reuse of this content should be sought from the publisher or the rights holder. This is the author created accepted manuscript following peer review and may differ slightly from the final published version. The final published version of this work is available at https://doi.org/10.1038/s41550-022-01619-w.en
dc.subjectQB Astronomyen
dc.subjectQC Physicsen
dc.subject3rd-DASen
dc.subject.lccQBen
dc.subject.lccQCen
dc.titleThe role of the cosmic web in the scatter of the galaxy stellar mass - gas metallicity relationen
dc.typeJournal articleen
dc.description.versionPostprinten
dc.contributor.institutionUniversity of St Andrews. School of Physics and Astronomyen
dc.identifier.doihttps://doi.org/10.1038/s41550-022-01619-w
dc.description.statusPeer revieweden
dc.date.embargoedUntil2022-09-14


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