Rubidium and Lead Abundances in Giant Stars of the Globular Clusters M4 and M5

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dc.contributor.authorYong, David
dc.contributor.authorLambert, David L
dc.contributor.authorPaulson, D.B.
dc.contributor.authorCarney, B W
dc.date.accessioned2015-12-08T22:10:20Z
dc.date.issued2008
dc.date.updated2015-12-08T07:31:31Z
dc.description.abstractWe present measurements of the neutron-capture elements Rb and Pb for bright giants in the globular clusters M4 and M5. The clusters are of similar metallicity ([Fe/H] ≃ -1.2), but M4 is decidedly s-process enriched relative to M5: [Ba/Fe] = +0.6 for M4
dc.identifier.issn0004-637X
dc.identifier.urihttp://hdl.handle.net/1885/29295
dc.publisherIOP Publishing
dc.sourceAstrophysical Journal, The
dc.subjectKeywords: Galaxy: abundances; Globular clusters: individual (M4, M5); Stars: abundances
dc.titleRubidium and Lead Abundances in Giant Stars of the Globular Clusters M4 and M5
dc.typeJournal article
local.bibliographicCitation.lastpage863
local.bibliographicCitation.startpage854
local.contributor.affiliationYong, David, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationLambert, David L, University of Texas
local.contributor.affiliationPaulson, D.B., NASA Goddard Space Flight Center
local.contributor.affiliationCarney, B W, University of North Carolina
local.contributor.authoruidYong, David, u3207952
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationu4362859xPUB64
local.identifier.citationvolume673
local.identifier.doi10.1086/524376
local.identifier.scopusID2-s2.0-40249110398
local.identifier.thomsonID000253454300019
local.type.statusPublished Version

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