Fig. 16.
Left panel: pseudo-entropy distribution scaled by r500. Right panel: distribution of Fe abundance versus the scaled pseudo-entropy of all the measured regions of the clusters: CIZA2242, 1RXSJ0603, A3376, A3667, A665 and A2256. The magenta dashed line is the best-fit linear model and the shaded area shows the 1σ uncertainties of the best-fit parameter. The cyan line and shadow are the results of Liu et al. (2018) for relaxed galaxy clusters.
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