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The Evolution of Copper in the Globular Cluster Omega Centauri

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dc.contributor.authorCunha, Katia
dc.contributor.authorSmith, Verne V
dc.contributor.authorSuntzeff, Nicholas B
dc.contributor.authorNorris, John
dc.contributor.authorDa Costa, Gary
dc.contributor.authorPlez, Bertrand
dc.date.accessioned2015-12-13T22:30:54Z
dc.date.issued2002
dc.date.updated2015-12-11T08:57:44Z
dc.description.abstractCopper abundances are presented for 40 red giant members of the massive Galactic globular cluster ω Centauri, as well as 15 red giant members of the globular clusters NGC 288, NGC 362, NGC 3201, NGC 6752, and M4 (NGC 6121). The spectra are of relatively
dc.identifier.issn0004-6256
dc.identifier.urihttp://hdl.handle.net/1885/75047
dc.publisherUniversity of Chicago Press
dc.sourceAstronomical Journal
dc.subjectKeywords: Globular clusters; Individual (? Centauri, NGC 288, NGC 362, NGC 3201, NGC 6752, M4)
dc.titleThe Evolution of Copper in the Globular Cluster Omega Centauri
dc.typeJournal article
local.bibliographicCitation.issue1
local.bibliographicCitation.lastpage388
local.bibliographicCitation.startpage379
local.contributor.affiliationCunha, Katia, Observatorio Nacional
local.contributor.affiliationSmith, Verne V, National Optical Astronomy Observatory
local.contributor.affiliationSuntzeff, Nicholas B, Cerro Tololo Inter-American Observatory
local.contributor.affiliationNorris, John, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationDa Costa, Gary, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationPlez, Bertrand, Universite Montpellier
local.contributor.authoruidNorris, John, u7401084
local.contributor.authoruidDa Costa, Gary, u9501331
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.description.refereedYes
local.identifier.absfor020104 - Galactic Astronomy
local.identifier.ariespublicationMigratedxPub4441
local.identifier.citationvolume124
local.identifier.doi10.1086/340967
local.identifier.scopusID2-s2.0-0011993676
local.type.statusPublished Version

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