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High-resolution observations in the near infrared show star clusters aroundthe active galactic nucleus (AGN) of the Seyfert 1 NGC2110, along with a 90 x35 pc bar of shocked gas material around its nucleus. These are seen for thefirst time in our imaging and gas kinematics of the central 100pc with the KeckOSIRIS instrument with adaptive optics. Each of these clusters is 2-3 timesbrighter than the Arches cluster close to the centre of the Milky Way. The corestar formation rate (SFR) is 0.3 M$_\odot$/yr. The photoionized gas (He I)dynamics imply an enclosed mass of 3-4 x 10$^8$ M$_\odot$. These observationsdemonstrate the physical linkage between AGN feedback, which triggers starformation in massive clusters, and the resulting stellar (and SNe) winds, whichcause the observed [Fe II] emission and feed the black hole.

Young Star Clusters In The Circumnuclear Region Of NGC 2110