The dynamics of the outer parts of ω Centauri

dc.contributor.author	Da Costa, Gary
dc.date.accessioned	2015-12-10T23:26:37Z
dc.date.issued	2012
dc.date.updated	2016-02-24T08:47:56Z
dc.description.abstract	The 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.issn	0004-637X
dc.identifier.uri	http://hdl.handle.net/1885/67841
dc.publisher	IOP Publishing
dc.rights	Author/s retain copyright	en_AU
dc.source	Astrophysical Journal, The
dc.subject	Keywords: globular clusters: general; globular clusters: individual (? Centauri, NGC 5139); stars: kinematics and dynamics
dc.title	The dynamics of the outer parts of ω Centauri
dc.type	Journal article
dcterms.accessRights	Open Access	en_AU
local.bibliographicCitation.issue	1
local.contributor.affiliation	Da Costa, Gary, College of Physical and Mathematical Sciences, ANU
local.contributor.authoruid	Da Costa, Gary, u9501331
local.description.notes	Imported from ARIES
local.identifier.absfor	020100 - ASTRONOMICAL AND SPACE SCIENCES
local.identifier.ariespublication	f5625xPUB1542
local.identifier.citationvolume	751
local.identifier.doi	10.1088/0004-637X/751/1/6
local.identifier.scopusID	2-s2.0-84860774381
local.identifier.thomsonID	000303814600006
local.type.status	Published Version

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