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ACCESS - IV. The quenching of star formation in a cluster population of dusty S0s

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dc.contributor.authorHaines, C. P.
dc.contributor.authorMerluzzi, Paola
dc.contributor.authorBusarello, Gianni
dc.contributor.authorDopita, Michael
dc.contributor.authorSmith, G. P.
dc.contributor.authorLa Barbera, F.
dc.contributor.authorGargiulo, A.
dc.contributor.authorRaychaudhury, Somak
dc.contributor.authorSmith, R. J.
dc.date.accessioned2015-12-10T21:57:32Z
dc.date.issued2011
dc.date.updated2016-02-24T09:54:08Z
dc.description.abstractWe present an analysis of the mid-infrared (MIR) colours of 165 70-μm-detected galaxies in the Shapley supercluster core (SSC) at z= 0.048 using panoramic Spitzer/MIPS 24- and 70-μm imaging. While the bulk of galaxies show f70/f24 colours typical of loc
dc.identifier.issn0035-8711
dc.identifier.urihttp://hdl.handle.net/1885/39819
dc.publisherBlackwell Publishing Ltd
dc.rightsAuthor/s retain copyrighten_AU
dc.sourceMonthly Notices of the Royal Astronomical Society
dc.subjectKeywords: Galaxies: clusters: general; Galaxies: clusters: individual: A3558; Galaxies: clusters: individual: A3562; Galaxies: evolution; Galaxies: star formation; Infrared: galaxies
dc.titleACCESS - IV. The quenching of star formation in a cluster population of dusty S0s
dc.typeJournal article
dcterms.accessRightsOpen Accessen_AU
local.bibliographicCitation.issue4
local.bibliographicCitation.lastpage2845
local.bibliographicCitation.startpage2831
local.contributor.affiliationHaines, C. P., Steward Observatory, University of Arizona
local.contributor.affiliationMerluzzi, Paola, INAF-Osservatorio Astronomico di Capodimonte
local.contributor.affiliationBusarello, Gianni, INAF-Osservatorio Astronomico di Capodimonte
local.contributor.affiliationDopita, Michael, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationSmith, G. P., University of Birmingham
local.contributor.affiliationLa Barbera, F, INAF - Osservatorio Astronomico di Capodimonte
local.contributor.affiliationGargiulo, A, INAF - Osservatorio Astronomico di Brera
local.contributor.affiliationRaychaudhury, Somak, University of Birmingham
local.contributor.affiliationSmith, R. J., University of Durham
local.contributor.authoruidDopita, Michael, u7501303
local.description.notesImported from ARIES
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.absseo970102 - Expanding Knowledge in the Physical Sciences
local.identifier.ariespublicationu3356449xPUB184
local.identifier.citationvolume417
local.identifier.doi10.1111/j.1365-2966.2011.19445.x
local.identifier.scopusID2-s2.0-80255138312
local.identifier.thomsonID000297043900029
local.type.statusPublished Version

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