Tracing the evolution in the iron content of the ICM

Details Tracing the evolution in the iron content of the ICM Tracing the evolution in the iron content of the ICM

2006-09-25

arxiv.org/abs/astro-ph/0609664v3

A&A 462, 429-442 (2007)

Astronomy and Astrophysics

Astrophysics

Astronomy and Astrophysics, Volume 462, Issue 2, February I 2007, pp. 429-442

Scientific paper

10.1051/0004-6361:20065568

We present a Chandra analysis of the X-ray spectra of 56 clusters of galaxies at z>0.3, which cover a temperature range 30.5. The emission weighted iron abundance is significantly higher (Z_{Fe}~0.4 Z_o) in the redshift range z~0.3-0.5, approaching the value measured locally in the inner 0.15 R_{vir} radii for a mix of cool-core and non cool-core clusters at 0.1

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