Table 4:

Results for the extended sample.

Abell cluster	Cool core		BCG	Large scale	VLBI	Ref.
		/yr
A400	N		3C 75A	WAT	one sided	White et al. (1997)
	N		3C 75B	WAT	one sided	White et al. (1997)
A407	N		UGC 2489	Tail rs	one sided	White et al. (1997)
A539	N		UGC 3274	radio quiet	n.d.	White et al. (1997)
A569	N	>	NGC 2329	WAT	one sided	White et al. (1997)
A576	N		CGCG 261-059	Tail rs	one sided	White et al. (1997)
A690	N		B2 0836+29 II	WAT	one sided	Giovannini et al. (2005); White et al. (1997)
A779	N		NGC 2832	radio quiet	n.d.	White et al. (1997)
A1185	N		NGC 3550	radio quiet	n.d.	White et al. (1997)
A1213	N		4C 29.41	FRI	one sided	White et al. (1997)
A1228	N	-	IC 2738	radio quiet	n.d.	-
A1314	N		IC 708	WAT	one sided	White et al. (1997)
	N		IC 712	small WAT	n.d.	White et al. (1997)
A1367	N		NGC 3842	small WAT	n.d.	White et al. (1997)
	N		3C 264	HT	one sided	Lara et al. (1999); White et al. (1997)
A1656	N		NGC 4874	small WAT	one sided	White et al. (1997)
A2147	N		UGC 10143	small WAT	n.d.	White et al. (1997)
A2151	N		NGC 6041	small WAT	core	White et al. (1997)
	N		NGC 6047	compact core+symmetric jets	n.d.	White et al. (1997)
A2162	N	-	NGC 6086	FRI, relic source	n.d.	-
A2197	N		NGC 6173	point source	one sided	White et al. (1997)
A2634	N		3C 465	WAT	one sided	Venturi et al. (1995); White et al. (1997)
A2666	N		NGC 7768	Tail rs	one sided	White et al. (1997)
A3526	N		PKS 1246-410	small tailed rs	one-sided	Hudson et al. (2010); Taylor et al. (2006b)
A262	Y		NGC 708	double-no core,jets	core	White et al. (1997)
A347	SCF		NGC 910	radio quiet	n.d.	White et al. (1997)
A426	Y		3C 84	Compact core+Halo	two sided	Taylor et al. (2006a); White et al. (1997)
A780	Y		Hydra A	double	two sided	Taylor (1996); White et al. (1997)
A1795	Y		4C 26.42	double	two sided	White et al. (1997); Liuzzo et al. (2009a)
A2052	Y		3C 317	bright core+halo (FRI)	two sided	Venturi et al. (2004); White et al. (1997)
A2152	Y		UGC 10187	Tail rs	n.d.	White et al. (1997)
A2199	Y		3C 338	double restarted	two sided	Feretti et al. (1993); White et al. (1997)
A2390	Y		B2151+174	MSO	two sided	Augusto et al. (2006); Allen et al. (2001)
A2597	Y		PKS 2322-123	asymmetric radiosource (FRI)	two sided	Taylor et al. (1999); Chen et al. (2007)

Notes. 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.