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dc.contributor.authorNordlander, T
dc.contributor.authorBessell, M S
dc.contributor.authorDa Costa, G S
dc.contributor.authorMackey, A D
dc.contributor.authorAsplund, M
dc.contributor.authorCasey, A R
dc.contributor.authorChiti, Anirudh
dc.contributor.authorEzzeddine, Rana
dc.contributor.authorFrebel, Anna L.
dc.contributor.authorLind, K
dc.contributor.authorMarino, A F
dc.contributor.authorMurphy, S J
dc.contributor.authorNorris, J E
dc.contributor.authorSchmidt, B P
dc.contributor.authorYong, D
dc.date.accessioned2020-10-28T20:49:05Z
dc.date.available2020-10-28T20:49:05Z
dc.date.issued2019-07
dc.date.submitted2019-06
dc.identifier.issn1745-3925
dc.identifier.issn1745-3933
dc.identifier.urihttps://hdl.handle.net/1721.1/128230
dc.description.abstractWe report the discovery of SMSS J160540.18−144323.1, a new ultra metal-poor halo star discovered with the SkyMapper telescope. We measure Fe/H = -6.2 ± 0.2 (1D LTE), the lowest ever detected abundance of iron in a star. The star is strongly carbon-enhanced, C/Fe = 3.9 ± 0.2$, while other abundances are compatible with an α-enhanced solar-like pattern with Ca/Fe = 0.4 ± 0.2, Mg/Fe = 0.6 ± 0.2, Ti/Fe = 0.8 ± 0.2, and no significant s- or r-process enrichment, Sr/Fe < 0.2 and Ba/Fe < 1.0 (3σ limits). Population III stars exploding as fallback supernovae may explain both the strong carbon enhancement and the apparent lack of enhancement of odd-Z and neutron-capture element abundances. Grids of supernova models computed for metal-free progenitor stars yield good matches for stars of about 10M[subscript⨀] imparting a low kinetic energy on the supernova ejecta, while models for stars more massive than roughly 20M[subscript⨀] are incompatible with the observed abundance pattern.en_US
dc.language.isoen
dc.publisherOxford University Press (OUP)en_US
dc.relation.isversionofhttp://dx.doi.org/10.1093/mnrasl/slz109en_US
dc.rightsCreative Commons Attribution-Noncommercial-Share Alikeen_US
dc.rights.urihttp://creativecommons.org/licenses/by-nc-sa/4.0/en_US
dc.sourcearXiven_US
dc.titleThe lowest detected stellar Fe abundance: the halo star SMSS J160540.18−144323.1en_US
dc.typeArticleen_US
dc.identifier.citationNordlander, T. et al. "The lowest detected stellar Fe abundance: the halo star SMSS J160540.18−144323.1." Monthly Notices of the Royal Astronomical Society: Letters 488, 1 (July 2019): L109–L113 © 2019 The Author(s)en_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Physicsen_US
dc.contributor.departmentMIT Kavli Institute for Astrophysics and Space Researchen_US
dc.relation.journalMonthly Notices of the Royal Astronomical Society: Lettersen_US
dc.eprint.versionOriginal manuscripten_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/NonPeerRevieweden_US
dc.date.updated2020-10-23T13:55:44Z
dspace.orderedauthorsNordlander, T; Bessell, MS; Da Costa, GS; Mackey, AD; Asplund, M; Casey, AR; Chiti, A; Ezzeddine, R; Frebel, A; Lind, K; Marino, AF; Murphy, SJ; Norris, JE; Schmidt, BP; Yong, Den_US
dspace.date.submission2020-10-23T13:55:52Z
mit.journal.volume488en_US
mit.journal.issue1en_US
mit.licenseOPEN_ACCESS_POLICY
mit.metadata.statusComplete


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