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A Spectroscopic Survey for ω Centauri Members at and beyond the Cluster Tidal Radius

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dc.contributor.authorDa Costa, Gary
dc.contributor.authorColeman, Matthew
dc.date.accessioned2015-12-08T22:30:27Z
dc.date.issued2008
dc.date.updated2016-02-24T11:05:59Z
dc.description.abstractWe have used the two-degree field (2dF) multi-fiber spectrograph of the Anglo-Australian Telescope (AAT) to search for candidate members of the unusual globular cluster ω Centauri at and beyond the cluster tidal radius. Velocities with an accuracy of 10
dc.identifier.issn0004-6256
dc.identifier.urihttp://hdl.handle.net/1885/34454
dc.publisherUniversity of Chicago Press
dc.sourceAstronomical Journal
dc.subjectKeywords: Galaxy: stellar content; Globular clusters: general; Globular clusters: individual (? Centauri, NGC 5139); Stars: kinematics
dc.titleA Spectroscopic Survey for ω Centauri Members at and beyond the Cluster Tidal Radius
dc.typeJournal article
local.bibliographicCitation.issue1
local.bibliographicCitation.lastpage517
local.bibliographicCitation.startpage506
local.contributor.affiliationDa Costa, Gary, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationColeman, Matthew, College of Physical and Mathematical Sciences, ANU
local.contributor.authoruidDa Costa, Gary, u9501331
local.contributor.authoruidColeman, Matthew, u4023418
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationu4362859xPUB113
local.identifier.citationvolume136
local.identifier.doi10.1088/0004-6256/136/1/506
local.identifier.scopusID2-s2.0-56449099503
local.identifier.thomsonID000257290200041
local.type.statusPublished Version

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