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Black holes and core expansion in massive star clusters

dc.contributor.authorMackey, Alasdair
dc.contributor.authorWilkinson, Mark, I.
dc.contributor.authorDavies, M B
dc.contributor.authorGilmore, Gerard
dc.date.accessioned2015-12-10T23:00:56Z
dc.date.issued2008
dc.date.updated2015-12-10T08:25:20Z
dc.description.abstractIn this study we present the results from realistic N-body modelling of massive star clusters in the Magellanic Clouds. We have computed eight simulations with N ∼ 105 particles; six of these were evolved for at least a Hubble time. The aim of this mode
dc.identifier.issn0035-8711
dc.identifier.urihttp://hdl.handle.net/1885/61554
dc.publisherBlackwell Publishing Ltd
dc.sourceMonthly Notices of the Royal Astronomical Society
dc.subjectKeywords: Globular clusters: general; Magellanic Clouds; Methods: N-body simulations; Stellar dynamics
dc.titleBlack holes and core expansion in massive star clusters
dc.typeJournal article
local.bibliographicCitation.issue1
local.bibliographicCitation.lastpage95
local.bibliographicCitation.startpage65
local.contributor.affiliationMackey, Alasdair, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationWilkinson, Mark, I. , University of Leicester
local.contributor.affiliationDavies, M B, Lund Observatory
local.contributor.affiliationGilmore, Gerard, University of Cambridge
local.contributor.authoruidMackey, Alasdair, u3208220
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.identifier.absfor020104 - Galactic Astronomy
local.identifier.ariespublicationU3488905xPUB620
local.identifier.citationvolume386
local.identifier.doi10.1111/j.1365-2966.2008.13052.x
local.identifier.scopusID2-s2.0-42449138407
local.identifier.thomsonID000255142500028
local.type.statusPublished Version

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