Abundances on the Main Sequence of ω Centauri

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dc.contributor.authorStanford, Laura
dc.contributor.authorDa Costa, Gary
dc.contributor.authorNorris, John
dc.contributor.authorCannon, Russell
dc.date.accessioned2015-12-07T22:30:28Z
dc.date.issued2007
dc.date.updated2015-12-07T10:05:02Z
dc.description.abstractAbundance ratios of carbon, nitrogen, and strontium relative to iron, calculated using spectrum synthesis techniques, are given for a sample of main-sequence and turnoff stars that belong to the globular cluster ω Centauri. The variations of carbon, nitr
dc.identifier.issn0004-637X
dc.identifier.urihttp://hdl.handle.net/1885/22334
dc.publisherIOP Publishing
dc.sourceAstrophysical Journal, The
dc.subjectKeywords: Globular clusters: general; Globular clusters: individual (? Centauri)
dc.titleAbundances on the Main Sequence of ω Centauri
dc.typeJournal article
local.bibliographicCitation.issue2
local.bibliographicCitation.lastpage929
local.bibliographicCitation.startpage911
local.contributor.affiliationStanford, Laura, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationDa Costa, Gary, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationNorris, John, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationCannon, Russell, Anglo-Australian Observatory
local.contributor.authoremailu9501331@anu.edu.au
local.contributor.authoruidStanford, Laura, u4014395
local.contributor.authoruidDa Costa, Gary, u9501331
local.contributor.authoruidNorris, John, u7401084
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.identifier.absfor020104 - Galactic Astronomy
local.identifier.ariespublicationu4193696xPUB21
local.identifier.citationvolume667
local.identifier.doi10.1086/520794
local.identifier.scopusID2-s2.0-35348906626
local.identifier.uidSubmittedByu4193696
local.type.statusPublished Version

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