\begin{table}%t3 \caption{\label{met_reg_tab}Properties of low entropy regions: clsters in Italics are ``AGN~CC-remnants'', while clusters in bold type are ``merger \mbox{CC-remnants}''.} %\centering \par \begin{tabular}{c c c} \hline\hline \noalign{\smallskip} Cluster & Metal abundance (solar) & BCG\tablefootmark{a} \\ \hline \it{A1650} & $0.397 \pm 0.021$ & Y \\ \it{MKW3s} & $0.459 \pm 0.009$ & Y \\ \it{A4038}\tablefootmark{b} & $0.402 \pm 0.008$ & Y \\ \it{A1644}\tablefootmark{b} & $0.703 \pm 0.049$ & Y \\ \bf{A1689} & $0.298 \pm 0.017$ & Y \\ \bf{A3558} & $0.350 \pm 0.010$ & Y \\ \bf{A576} & $0.520 \pm 0.035$ & Y \\ \bf{A754} & $0.314 \pm 0.021$ & N\tablefootmark{c}\\ \bf{A3562} & $0.471 \pm 0.021$ & Y \\ \bf{A3571} & $0.349 \pm 0.013$ & Y \\ \bf{A3667} & $0.327 \pm 0.012$ & N \\ \bf{A2256} & $0.351 \pm 0.038$ & N \\ A2319 & $0.242 \pm 0.012$ & Y \\ A3266 & $0.232 \pm 0.039$& Y \\ A399 & $0.221 \pm 0.053$ & Y \\ A401 & $0.262 \pm 0.044$ & N \\ A3158 & $ 0.275 \pm 0.077$ & N \\ A119 & $0.242 \pm 0.078$ & N \\ A2255\tablefootmark{d} & $0.547 \pm 0.224$ & \\ A3532\tablefootmark{d} & $0.473 \pm 0.095$ & \\ Triangulum Australis\tablefootmark{d} & $0.369 \pm 0.151$ & \\ \hline \end{tabular} \tablefoot {\tablefoottext{a}{``Y'' if the BCG is found in the low-entropy region and ``N''~if it is elsewhere.} \tablefoottext{b}{even if the central entropy of this cluster is within the reach of AGN~outbursts, it~also shows some indications of on-going interaction and cannot be unambiguously associated to the ``AGN~\mbox{CC-remnant} class'' (see~text).} \tablefoottext{c}{The BCG 2MASSX~J09083238-0937470 is not associated to the \mbox{CC-remnant}, which however coincides with the position of the elliptical galaxy 2MASSX~J09091923-0941591.} \tablefoottext{d}{Due to the large indetermination of the metal abundance estimate, we could not unambiguously detect or exclude the presence of a metal abundance excess in this~object.}} \end{table}