\begin{table}%T4 \par \caption{\label{tab4}Results for the extended sample.} \small%\centering \par \begin{tabular}{ccccccc} \hline \hline\noalign{\smallskip} Abell cluster&Cool core&$M_{\rm accr}$&BCG&Large scale&VLBI&Ref.\\ & & $M_{\odot}$/yr& & & \\ \hline A400 &N &$0.0^{\rm +28.3}_{-0.0}$&3C~75A &WAT &one sided&\citet{whi97}\\ &N &$0.0^{\rm +28.3}_{-0.0}$&3C~75B &WAT &one sided&\citet{whi97}\\ A407 &N &$4.6^{\rm +11.8}_{-4.6}$&UGC~2489 &Tail rs &one sided&\citet{whi97}\\ A539 &N &$2.1^{\rm +6.8}_{-2.1}$&UGC~3274 &radio quiet & n.d.&\citet{whi97}\\ A569 &N &$>$$5.2^{\rm +0.0}_{->4.2}$&NGC~2329 &WAT &one sided&\citet{whi97}\\ A576 &N &$17^{\rm +47}_{-17}$&CGCG~261-059 &Tail rs &one sided&\citet{whi97}\\ A690 &N &$0.0^{\rm +15.3}_{-0.0}$&B2 0836+29 II &WAT &one sided&\citet{gio05,whi97}\\ A779 &N &$3.1^{\rm +1.1}_{-1.1}$&NGC~2832 &radio quiet &n.d.&\citet{whi97}\\ A1185 &N &$0.0^{\rm +1.5}_{-0.0}$&NGC~3550 &radio quiet &n.d.&\citet{whi97}\\ A1213 &N &$0.0^{\rm +11.5}_{-0.0}$&4C~29.41 & FRI &one sided&\citet{whi97}\\ A1228 &N &-- &IC~2738 &radio quiet &n.d.&--\\ A1314 &N &$0.0^{\rm +3.0}_{-0.0}$&IC~708 &WAT&one sided&\citet{whi97}\\ &N &$0.0^{\rm +3.0}_{-0.0}$&IC~712 &small WAT &n.d.&\citet{whi97}\\ A1367 &N &$2.3^{\rm +6.8}_{-2.3}$&NGC~3842 &small WAT &n.d.&\citet{whi97}\\ &N &$2.3^{\rm +6.8}_{-2.3}$&3C~264 &HT &one sided&\citet{la99,whi97}\\ A1656 &N &$0.0^{\rm +1.0}_{-0.0}$&NGC~4874 &small WAT &one sided&\citet{whi97}\\ A2147 &N &$0.0^{\rm +14.5}_{-0.0}$&UGC~10143 &small WAT & n.d.&\citet{whi97}\\ A2151 &N &$6.3^{\rm +26.3}_{-3.2}$&NGC~6041 &small WAT &core&\citet{whi97}\\ &N &$6.3^{\rm +26.3}_{-3.2}$&NGC~6047 &compact core+symmetric jets&n.d.&\citet{whi97}\\ A2162 &N &-- &NGC~6086 &FRI, relic source &n.d.&--\\ A2197 &N &$2.4^{\rm +3.0}_{-2.4}$&NGC~6173 &point source &one sided&\citet{whi97}\\ A2634 &N &$0.0^{\rm +1.5}_{-0.0}$&3C~465 &WAT &one sided&\citet{ve95,whi97}\\ A2666 &N &$0.0^{\rm +2.6}_{-0.0}$&NGC~7768 &Tail rs &one sided&\citet{whi97}\\ A3526 &N &$5.2^{\rm +0.3}_{-0.3}$&PKS 1246-410 &small tailed rs&one-sided&\citet{tas06, hud09}\\ \\ A262 & Y &$9.4^{\rm +21.2}_{-4.4}$&NGC~708 &double-no core,jets &core&\citet{whi97}\\ A347 &SCF &$7.8^{\rm +3.5}_{-2.7}$&NGC~910 &radio quiet &n.d.&\citet{whi97}\\ A426 &Y &$291^{\rm +>-7}_{-58}$&3C~84 &Compact core+Halo& two sided&\citet{tay06,whi97}\\ A780 &Y &$222^{\rm +98}_{-132}$&Hydra A &double &two sided&\citet{tay96,whi97}\\ A1795&Y &$321^{\rm +166}_{-213}$&4C~26.42 &double &two sided&\citet{liu09,whi97}\\ A2052&Y &$94^{\rm +84}_{-37}$&3C~317 &bright core+halo (FRI)&two sided&\citet{ve04,whi97}\\ A2152& Y&$20^{\rm +13}_{-20}$&UGC~10187 &Tail rs&n.d.&\citet{whi97}\\ A2199&Y &$97^{\rm +9}_{-31}$&3C~338 &double restarted&two sided&\citet{whi97,fe93}\\ A2390&Y &$247^{\rm +43}_{-91}$&B2151+174 &MSO&two sided&\citet{au06, all01}\\ A2597&Y &$501^{\rm +58}_{-512}$ &PKS 2322-123 &asymmetric radiosource (FRI)& two sided&\citet{tay99,che07}\\ \hline \end{tabular} \tablefoot{In the first column, we report the Abell cluster of BCG of our sample, in Col.~2, we indicate~Y if the Abell cluster shows a cool core, N~if it doesn't, in Col.~3 there are the value of central mass accretion rate of the cluster taken from the literature, in Col.~4 there are the names of BCGs. Column~5 is for the large scale morphology of the BCG: we use WAT for Wide Angle Tail radiosource, HT for head tail radiosource, MSO for medium symmetric source. In Col.~6, we mark the parsec-scale structure: one sided, two sided, core (unresolved) or n.d. for the non detections. In the last column, we give the references for the mas scale structure when the source is yet well studied at mas scale in literature and for values of mass accretion rate given in Col.~3. } \end{table}