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The physical nature of the X-ray/radio correlation of AGN is still anunsolved question. High angular resolution observations are necessary todisentangle the associated energy dynamics into nuclear and stellar components.We present MERLIN/EVN 18cm observations of 13 X-raying AGN. The sample consistsof Seyfert 1, Narrow Line Seyfert 1, and LINER-like galaxies. We find that forall objects the radio emission is unresolved and that the radio luminositiesand brightness temperatures are too high for star formation to play animportant role. This indicates that the radio emission in these sources isclosely connected to processes that occur in the vicinity of the centralmassive black hole, also where the X-ray emission is believed to originate in.

The nuclear radio structure of X-ray bright AGN