4.6 Article

Thermo-dynamic and chemical properties of the intra-cluster medium

Journal

ASTRONOMY & ASTROPHYSICS
Volume 510, Issue -, Pages -

Publisher

EDP SCIENCES S A
DOI: 10.1051/0004-6361/200913094

Keywords

X-rays: galaxies: clusters; galaxies: clusters: general; galaxies: abundances

Funding

  1. ASI-INAF [I/023/05/0, I/088/06/0]

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Aims. We aim to provide constraints on evolutionary scenarios in clusters. One of our main goals is to understand whether, as claimed by some, the cool core/non-cool core division is established once and for all during the early history of a cluster. Methods. We employ a sample of similar or equal to 60 objects to classify clusters according to different properties. We characterize cluster cores in terms of their thermo-dynamic and chemical properties and clusters as a whole in terms of their dynamical properties. Results. We find that I) the vast majority of merging systems feature high-entropy cores (HEC) and II) objects with lower entropy cores feature more pronounced metallicity peaks than objects with higher entropy cores. We identify a small number of medium (MEC) and high (HEC) entropy core systems that, unlike most other such objects, feature a high central metallicity. The majority of these outliers are mergers, i.e. systems far from their equilibrium configuration. Conclusions. We surmise that medium (MEC) and high (HEC) entropy core systems with a high central metallicity have recently evolved from low-entropy core (LEC) clusters that have experienced a heating event associated to AGN or merger activity.

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