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dc.contributor.authorAde, Peter Anthony Robert
dc.contributor.authorBarreiro Vilas, Rita Belén 
dc.contributor.authorDiego Rodríguez, José María 
dc.contributor.authorGonzález-Nuevo González, Joaquín
dc.contributor.authorHerranz Muñoz, Diego 
dc.contributor.authorLópez-Caniego Alcarria, Marcos
dc.contributor.authorMartínez González, Enrique
dc.contributor.authorToffolatti, Luigi
dc.contributor.authorVielva Martínez, Patricio 
dc.contributor.otherUniversidad de Cantabriaes_ES
dc.date.accessioned2023-05-11T11:03:46Z
dc.date.available2023-05-11T11:03:46Z
dc.date.issued2013
dc.identifier.issn0004-6361
dc.identifier.issn1432-0746
dc.identifier.urihttps://hdl.handle.net/10902/28841
dc.description.abstractThe survey of galaxy clusters performed by Planck through the Sunyaev-Zeldovich effect has already discovered many interesting objects, thanks to its full sky coverage. One of the SZcandidates detected in the early months of the mission near to the signal-to-noise threshold, PLCKG214.6+37.0, was later revealed by XMM-Newton to be a triple system of galaxy clusters. We present the results from a deep XMM-Newton re-observation of PLCKG214.6+37.0, part of a multi-wavelength programme to investigate Planck discovered superclusters. The characterisation of the physical properties of the three components has allowed us to build a template model to extract the total SZ signal of this system with Planck data. We have partly reconciled the discrepancy between the expected SZ signal derived from X-rays and the observed one, which are now consistent within 1.2?. We measured the redshift of the three components with the iron lines in the X-ray spectrum, and confirm that the three clumps are likely part of the same supercluster structure. The analysis of the dynamical state of the three components, as well as the absence of detectable excess X-ray emission, suggests that we are witnessing the formation of a massive cluster at an early phase of interaction.es_ES
dc.format.extent14 p.es_ES
dc.language.isoenges_ES
dc.publisherEDP Scienceses_ES
dc.rights© ESO 2013es_ES
dc.sourceAstronomy & Astrophysics, 2013, 550, A132es_ES
dc.subject.otherGalaxies: clusters: generales_ES
dc.subject.otherLarge-scale structure of Universees_ES
dc.subject.otherGalaxies: clusters: individual: PLCKG214.6+37.0es_ES
dc.titlePlanck intermediate results VI. The dynamical structure of PLCKG214.6+37.0, a Planck discovered triple system of galaxy clusterses_ES
dc.typeinfo:eu-repo/semantics/articlees_ES
dc.relation.publisherVersionhttps://doi.org/10.1051/0004-6361/201220039es_ES
dc.rights.accessRightsopenAccesses_ES
dc.identifier.DOI10.1051/0004-6361/201220039
dc.type.versionpublishedVersiones_ES


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