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

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dc.contributor.authorStanford, Laura
dc.contributor.authorDa Costa, Gary
dc.contributor.authorNorris, John
dc.date.accessioned2015-12-08T22:37:59Z
dc.date.issued2010
dc.date.updated2016-02-24T09:53:45Z
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.identifier.issn0004-637X
dc.identifier.urihttp://hdl.handle.net/1885/35753
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.bibliographicCitation.issue2
local.bibliographicCitation.lastpage1014
local.bibliographicCitation.startpage1001
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.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.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationu3356449xPUB128
local.identifier.citationvolume714
local.identifier.doi10.1088/0004-637X/714/2/1001
local.identifier.scopusID2-s2.0-77951684304
local.identifier.thomsonID000276973100002
local.type.statusPublished Version

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