Temperature structure of the intergalactic medium within seven nearby and bright clusters of galaxies observed with XMM-Newton

2007/12/04 by H. Bourdin, P. Mazzotta · 4 citations
Physics and Astronomy · #Astronomy and Astrophysical Research #Galaxies: Formation, Evolution, Phenomena #Stellar, planetary, and galactic studies #astro-ph

paper · pdf · doi:10.1051/0004-6361:20065758

published as Astron.Astrophys.479:3078,2008 · published in A&A

openalex publication_date 2007/12/04 · arxiv created 2008/02/13 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/01

Abstract

Aims.Using a newly developed algorithm, we map, to the highest angular resolution allowed by the data, the temperature structure of the intra-cluster medium (ICM) within a nearly complete X-ray flux limited sample of galaxy clusters in the redshift range between and . Our sample contains seven bright clusters of galaxies observed with XMM-Newton: Abell 399, Abell 401, Abell 478, Abell 1795, Abell 2029, Abell 2065, Abell 2256.

Citations

• Collisional Plasma Models with APEC/APED: Emission-Line Diagnostics of Hydrogen-like and Helium-like Ions
• AnXMM-Newtonobservation of the dynamically active binary cluster A1750
• H I in the Galaxy
• Adaptive spatial binning of integral-field spectroscopic data using Voronoi tessellations
• A multiscale vision model adapted to the astronomical images
• ChandraTemperature Profiles for a Sample of Nearby Relaxed Galaxy Clusters
• De-noising by soft-thresholding
• XMM-Newtonobservation of the relaxed cluster A478: Gas and dark matter distribution from 0.01R₂00 to 0.5R\mathsf₂₀₀
• Deep inside the core of Abell 1795: theChandraview

Cited by

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• Gas sloshing, cold front formation and metal redistribution: the Virgo cluster as a quantitative test case
• The mergers in Abell 2256: displaced gas and its connection to the radio-emitting plasma
• Exploring the multiphase medium in MKW 08: from the central active galaxy up to cluster scales

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• Galaxy cluster temperature maps from joint X-ray and SZ maps with The Three Hundred hydrodynamical simulations