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    Planck intermediate results VI. The dynamical structure of PLCKG214.6+37.0, a Planck discovered triple system of galaxy clusters

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    Identificadores
    URI: https://hdl.handle.net/10902/28841
    DOI: 10.1051/0004-6361/201220039
    ISSN: 0004-6361
    ISSN: 1432-0746
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    Autoría
    Ade, Peter Anthony Robert; Barreiro Vilas, Rita BelénAutoridad Unican; Diego Rodríguez, José MaríaAutoridad Unican; González-Nuevo González, Joaquín; Herranz Muñoz, DiegoAutoridad Unican; López-Caniego Alcarria, Marcos; Martínez González, Enrique; Toffolatti, Luigi; Vielva Martínez, PatricioAutoridad Unican
    Fecha
    2013
    Derechos
    © ESO 2013
    Publicado en
    Astronomy & Astrophysics, 2013, 550, A132
    Editorial
    EDP Sciences
    Enlace a la publicación
    https://doi.org/10.1051/0004-6361/201220039
    Palabras clave
    Galaxies: clusters: general
    Large-scale structure of Universe
    Galaxies: clusters: individual: PLCKG214.6+37.0
    Resumen/Abstract
    The 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.
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    UNIVERSIDAD DE CANTABRIA

    Repositorio realizado por la Biblioteca Universitaria utilizando DSpace software
    Contacto | Sugerencias
    Metadatos sujetos a:licencia de Creative Commons Reconocimiento 4.0 España