  We present X-ray (Chandra), radio (EVLA and EVN), and archival optical data
of the triple-merging system in NGC3341. Our panchromatic analysis confirms the
presence of a Seyfert 2 AGN in NGC3341B, one of the secondary dwarf companions.
On the other hand, the nucleus of the primary galaxy, consistent with a
star-forming region of a few solar masses per year, and NGC3341C are very
unlikely to host an AGN. We therefore suggest that NGC3341 is an exceptional
example of an AGN triggered in the satellite galaxy of a minor-merging system.
The existence of such a system can have important implications in the models of
hierarchical growth of structures. Further observational and theoretical
efforts on NGC3341 and potentially similar sources are needed in order to
understand the role of minor mergers on the onset of AGN activity, and in the
evolution of massive galaxies.
