The dynamics of the outer parts of ω Centauri

dc.contributor.authorDa Costa, Gary
dc.date.accessioned2015-12-10T23:26:37Z
dc.date.issued2012
dc.date.updated2016-02-24T08:47:56Z
dc.description.abstractThe multi-object fiber-fed spectrograph AAOmega at the Anglo-Australian Telescope has been used to establish and measure accurate (≤1kms-1) radial velocities for a new sample of members in the outer parts of the stellar system ω Centauri. The new sampl
dc.identifier.issn0004-637X
dc.identifier.urihttp://hdl.handle.net/1885/67841
dc.publisherIOP Publishing
dc.rightsAuthor/s retain copyrighten_AU
dc.sourceAstrophysical Journal, The
dc.subjectKeywords: globular clusters: general; globular clusters: individual (? Centauri, NGC 5139); stars: kinematics and dynamics
dc.titleThe dynamics of the outer parts of ω Centauri
dc.typeJournal article
dcterms.accessRightsOpen Accessen_AU
local.bibliographicCitation.issue1
local.contributor.affiliationDa Costa, Gary, College of Physical and Mathematical Sciences, ANU
local.contributor.authoremailu9501331@anu.edu.au
local.contributor.authoruidDa Costa, Gary, u9501331
local.description.notesImported from ARIES
local.identifier.absfor020100 - ASTRONOMICAL AND SPACE SCIENCES
local.identifier.ariespublicationf5625xPUB1542
local.identifier.citationvolume751
local.identifier.doi10.1088/0004-637X/751/1/6
local.identifier.scopusID2-s2.0-84860774381
local.identifier.thomsonID000303814600006
local.identifier.uidSubmittedByf5625
local.type.statusPublished Version

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