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dc.contributor.authorIshigaki, Miho N.
dc.contributor.authorTominaga, Nozomu
dc.contributor.authorKobayashi, Chiaki
dc.contributor.authorNomoto, Ken'ichi
dc.date.accessioned2017-09-13T15:57:01Z
dc.date.available2017-09-13T15:57:01Z
dc.date.issued2014-08-26
dc.identifier.citationIshigaki , M N , Tominaga , N , Kobayashi , C & Nomoto , K 2014 , ' Faint Population III supernovae as the origin of the most iron-poor stars ' , Astrophysical Journal Letters , vol. 792 , no. 2 . https://doi.org/10.1088/2041-8205/792/2/L32
dc.identifier.issn2041-8205
dc.identifier.otherPURE: 10327434
dc.identifier.otherPURE UUID: a87e1756-cb12-41a1-9de8-eba8a31db437
dc.identifier.otherArXiv: http://arxiv.org/abs/1404.4817v3
dc.identifier.otherScopus: 84906908815
dc.identifier.urihttp://hdl.handle.net/2299/19372
dc.descriptionThe Astrophysical Journal Letters, 792:L32 (6pp), 2014 September 10. doi: 10.1088/2041-8205/792/2/L32. © 2014 The American Astronomical Society. All rights reserved. Printed in the U.S.A.
dc.description.abstractThe most iron-deficient stars in the Milky Way provide important observational constraints on the nature of astrophysical objects that have enriched the primordial gas with heavy elements from which these stars were formed. Among them, the recently discovered iron-deficient star SMSS J031300.36-670839.3 shows a remarkable chemical composition with non-detection of iron ([Fe/H]$ H]$en
dc.format.extent6
dc.language.isoeng
dc.relation.ispartofAstrophysical Journal Letters
dc.rightsOpen
dc.subjectstars: abundances
dc.subjectstars: Population III
dc.subjectsupernovae: general
dc.titleFaint Population III supernovae as the origin of the most iron-poor starsen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionScience & Technology Research Institute
dc.contributor.institutionCentre for Astrophysics Research
dc.description.statusPeer reviewed
dc.relation.schoolSchool of Physics, Astronomy and Mathematics
dc.description.versiontypeFinal Published version
dcterms.dateAccepted2014-08-26
rioxxterms.versionAM
rioxxterms.versionVoR
rioxxterms.versionofrecordhttps://doi.org/10.1088/2041-8205/792/2/L32
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue
herts.rights.accesstypeOpen


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