Cool gas in the core of the Centaurus cluster

Physics

Scientific paper

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Scientific paper

I will present results from a recent paper, where, with a deep XMM RGS observation of the Centaurus cluster, we manage to detect X-ray emitting material a factor of 10 colder in temperature than in the cluster outskirts. The Fe XVII emission lines are directly seen in the spectrum. In addition I will show XMM RGS results from a new sample of clusters ranging in mass scale, including HCG 62, A1835, A262 and PKS1404.

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