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Abundances of C, N, Sr, and Ba on the Red Giant Branch of ω Centauri

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Stanford, Laura; Da Costa, Gary; Norris, John

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Abundances relative to iron for carbon, nitrogen, strontium, and barium are presented for 33 stars on the red giant branch (RGB) of the globular cluster ω Centauri. They are based on intermediate-resolution spectroscopic data covering the blue spectral r

dc.contributor.authorStanford, Laura
dc.contributor.authorDa Costa, Gary
dc.contributor.authorNorris, John
dc.date.accessioned2015-12-08T22:37:59Z
dc.identifier.issn0004-637X
dc.identifier.urihttp://hdl.handle.net/1885/35753
dc.description.abstractAbundances relative to iron for carbon, nitrogen, strontium, and barium are presented for 33 stars on the red giant branch (RGB) of the globular cluster ω Centauri. They are based on intermediate-resolution spectroscopic data covering the blue spectral r
dc.publisherIOP Publishing
dc.sourceAstrophysical Journal, The
dc.subjectKeywords: Globular clusters: general; Globular clusters: individual (? Centauri)
dc.titleAbundances of C, N, Sr, and Ba on the Red Giant Branch of ω Centauri
dc.typeJournal article
local.description.notesImported from ARIES
local.identifier.citationvolume714
dc.date.issued2010
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationu3356449xPUB128
local.type.statusPublished Version
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.description.embargo2037-12-31
local.bibliographicCitation.issue2
local.bibliographicCitation.startpage1001
local.bibliographicCitation.lastpage1014
local.identifier.doi10.1088/0004-637X/714/2/1001
dc.date.updated2016-02-24T09:53:45Z
local.identifier.scopusID2-s2.0-77951684304
local.identifier.thomsonID000276973100002
CollectionsANU Research Publications

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