\begin{table}%t4
\par
\caption {Properties of the extended radio emission regions in the
cluster centre.\label{tab:unassociated}}
%\centerline
 {\begin{tabular}{llllll}
\hline\hline
\noalign{\smallskip}
ID & 8.6 GHz & 4.8 GHz &2.5 GHz & Spec. Index & Assoc.\\
&(mJy)&(mJy)&(mJy)&&Star\\
\hline
A1 &  5.6 &  7.6 &  7.6 &$-0.24\pm0.15$  & D09-R1\\
A2 & 23.8 & 26.0 & 35.5 &$-0.32\pm0.10$  & WR~B\\
A3 & 12.1 & 11.1 & 16.0 &$-0.23\pm0.20$  & W20 \\
A4 &  3.5 &  4.7 &  5.5 &$-0.36\pm0.10$  & \\
A5 &  2.0 &  1.9 &  2.0 &$-0.01\pm0.11$  & \\
A6 & 71.9 & 78.0 & 81.8 &$-0.05\pm0.07$  & \\
A7 & 22.4 & 28.2 & 27.0 &$-0.14\pm0.13$  & W9\\
A8 &153.3 &164.9 &161.4 &$-0.04\pm0.11$  & W26\\
Total&295&322&337&&\\
\hline
\end{tabular}}
\tablefoot {These fluxes are for the extended emission only in these
regions. The fluxes of the radio stars in these regions has been
subtracted. The flux uncertainty is assumed to be $\sim$$10\%$.}
\end{table}