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The A2667 giant arc at z = 1.03: Evidence for large-scale shocks at high redshift

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dc.contributor.authorYuan, T.-T.
dc.contributor.authorKewley, Lisa
dc.contributor.authorSwinbank, A M
dc.contributor.authorRichard, J
dc.date.accessioned2015-12-10T23:31:25Z
dc.date.issued2012
dc.date.updated2016-02-24T08:50:35Z
dc.description.abstractWe present the spatially resolved emission line ratio properties of a ∼ 1010 M⊙ star-forming galaxy at redshift z = 1.03. This galaxy is gravitationally lensed as a triple-image giant arc behind the massive lensing cluster A2667. The main image of the
dc.identifier.issn0004-637X
dc.identifier.urihttp://hdl.handle.net/1885/68617
dc.publisherIOP Publishing
dc.rightsAuthor/s retain copyrighten_AU
dc.sourceAstrophysical Journal, The
dc.subjectKeywords: galaxies: abundances; galaxies: evolution; galaxies: high-redshift; gravitational lensing: strong; ISM: jets and outflows
dc.titleThe A2667 giant arc at z = 1.03: Evidence for large-scale shocks at high redshift
dc.typeJournal article
dcterms.accessRightsOpen Accessen_AU
local.bibliographicCitation.issue66
local.bibliographicCitation.lastpage11
local.bibliographicCitation.startpage1
local.contributor.affiliationYuan, T.-T., University of Hawaii
local.contributor.affiliationKewley, Lisa, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationSwinbank, A M, Durham University
local.contributor.affiliationRichard, J, Universite Lyon 1
local.contributor.authoruidKewley, Lisa, u9415124
local.description.notesImported from ARIES
local.identifier.absfor020103 - Cosmology and Extragalactic Astronomy
local.identifier.ariespublicationf5625xPUB1776
local.identifier.ariespublicationu4630950xPUB179
local.identifier.citationvolume759
local.identifier.doi10.1088/0004-637X/759/1/66
local.identifier.scopusID2-s2.0-84868130493
local.identifier.thomsonID000310566900066
local.type.statusPublished Version

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