Fig. 8.
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Fe abundance versus entropy for cool core clusters. Abundance measurements are taken from Leccardi et al. (2010), they have been converted to Asplund et al. (2009) solar abundances. Entropy measurements come from the ACCEPT archive of Chandra data (Cavagnolo et al. 2009). The sample comprises the 12 cool core systems identified in Leccardi et al. (2010) for which adequate entropy measurements could be found in ACCEPT.
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