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Angular momenta, dynamical masses, and mergers of brightest cluster galaxies

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dc.contributor.authorJimmy, .
dc.contributor.authorTran, Kim-Vy
dc.contributor.authorBrough, Sarah
dc.contributor.authorGebhardt, Karl
dc.contributor.authorLinden, Anja von der
dc.contributor.authorCouch, Warrick
dc.contributor.authorSharp, Robert
dc.date.accessioned2015-12-13T22:32:27Z
dc.date.issued2013
dc.date.updated2015-12-11T09:07:25Z
dc.description.abstractUsing the VIMOS integral field unit (IFU) spectrograph on the Very Large Telescope, we have spatially mapped the kinematic properties of 10 nearby brightest cluster galaxies (BCGs) and 4 BCG companion galaxies located within a redshift of z = 0.1. In the
dc.identifier.issn0004-637X
dc.identifier.urihttp://hdl.handle.net/1885/75568
dc.publisherIOP Publishing
dc.rightsAuthor/s retain copyrighten_AU
dc.sourceAstrophysical Journal, The
dc.titleAngular momenta, dynamical masses, and mergers of brightest cluster galaxies
dc.typeJournal article
dcterms.accessRightsOpen Accessen_AU
local.bibliographicCitation.issue2
local.bibliographicCitation.startpage12
local.contributor.affiliationJimmy, ., Texas A&M University
local.contributor.affiliationTran, Kim-Vy, Texas A&M University
local.contributor.affiliationBrough, Sarah, Australian Astronomical Observatory
local.contributor.affiliationGebhardt, Karl, University of Texas at Austin
local.contributor.affiliationLinden, Anja von der, Stanford University
local.contributor.affiliationCouch, Warrick, Swinburne University of Technology
local.contributor.affiliationSharp, Robert, College of Physical and Mathematical Sciences, ANU
local.contributor.authoruidSharp, Robert, u4954956
local.description.notesImported from ARIES
local.identifier.absfor020100 - ASTRONOMICAL AND SPACE SCIENCES
local.identifier.ariespublicationf5625xPUB4679
local.identifier.citationvolume778
local.identifier.doi10.1088/0004-637X/778/2/171
local.identifier.scopusID2-s2.0-84887923999
local.identifier.thomsonID000327762800086
local.type.statusPublished Version

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