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The oxygen abundance of the ultra-metal-poor star HE 0557-4840

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dc.contributor.authorNorris, John
dc.contributor.authorChristlieb, N
dc.contributor.authorBessell, Michael
dc.contributor.authorAsplund, Martin
dc.contributor.authorEriksson, K.
dc.contributor.authorKorn, A. J.
dc.date.accessioned2015-12-10T23:06:53Z
dc.date.issued2012
dc.date.updated2016-02-24T09:34:52Z
dc.description.abstractWe present a high-resolution ultraviolet (UV) spectrum of the ultra-metal-poor (UMP) carbon-enhanced red giant HE 0557-4840 (Teff/log g/[Fe/H] = 4900/2.2/-4.8). Combining these data with earlier observations, the radial velocity is 212.0 ± 0.4kms-1, with
dc.identifier.issn0004-637X
dc.identifier.urihttp://hdl.handle.net/1885/62854
dc.publisherIOP Publishing
dc.rightsAuthor/s retain copyrighten_AU
dc.sourceAstrophysical Journal, The
dc.subjectKeywords: early universe; Galaxy: formation; Galaxy: halo; nuclear reactions, nucleosynthesis, abundances; stars: abundances; stars: individual (HE 0557-4840)
dc.titleThe oxygen abundance of the ultra-metal-poor star HE 0557-4840
dc.typeJournal article
dcterms.accessRightsOpen Accessen_AU
local.bibliographicCitation.issue2
local.bibliographicCitation.startpage150
local.contributor.affiliationNorris, John, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationChristlieb, N, University of Heidelberg
local.contributor.affiliationBessell, Michael, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationAsplund, Martin, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationEriksson, K., Uppsala University
local.contributor.affiliationKorn, A. J., Uppsala University
local.contributor.authoruidNorris, John, u7401084
local.contributor.authoruidBessell, Michael, u6900904
local.contributor.authoruidAsplund, Martin, u4042723
local.description.notesImported from ARIES
local.identifier.absfor020100 - ASTRONOMICAL AND SPACE SCIENCES
local.identifier.ariespublicationf5625xPUB744
local.identifier.citationvolume753
local.identifier.doi10.1088/0004-637X/753/2/150
local.identifier.scopusID2-s2.0-84862870629
local.identifier.thomsonID000305912700057
local.type.statusPublished Version

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