The Spectroscopic Age of 47 Tucanae

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dc.contributor.authorGibson, Brad K
dc.contributor.authorMadgwick, Darren
dc.contributor.authorJones, L
dc.contributor.authorDa Costa, Gary
dc.contributor.authorNorris, John
dc.date.accessioned2015-12-13T23:40:26Z
dc.date.available2015-12-13T23:40:26Z
dc.date.issued1999
dc.date.updated2015-12-12T09:29:08Z
dc.description.abstractHigh signal-to-noise ratio integrated spectra of the metal-rich globular cluster 47 Tuc, spanning the HγHR and Fe 4668 line indices, have been obtained. Jones & Worthey have suggested that the combination of these indices is the best available mechanism
dc.identifier.issn0004-6256
dc.identifier.urihttp://hdl.handle.net/1885/94468
dc.publisherUniversity of Chicago Press
dc.sourceAstronomical Journal
dc.subjectKeywords: Galaxies: abundances; Galaxies: elliptical and lenticular, cD; Globular clusters : individual (47 Tucanae); Stars : abundances
dc.titleThe Spectroscopic Age of 47 Tucanae
dc.typeJournal article
local.bibliographicCitation.lastpage1272
local.bibliographicCitation.startpage1268
local.contributor.affiliationGibson, Brad K, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationMadgwick, Darren, University of California
local.contributor.affiliationJones, L, LIGO - California Institute of Technology
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.authoruidGibson, Brad K, v003767
local.contributor.authoruidDa Costa, Gary, u9501331
local.contributor.authoruidNorris, John, u7401084
local.description.notesImported from ARIES
local.description.refereedYes
local.identifier.absfor020104 - Galactic Astronomy
local.identifier.ariespublicationMigratedxPub24064
local.identifier.citationvolume118
local.identifier.scopusID2-s2.0-0007020174
local.type.statusPublished Version

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