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We investigated the interstellar medium (ISM) properties in the centralregions of nearby Seyfert galaxies characterised by prominent conical orbi-conical outflows belonging to the MAGNUM survey by exploiting theunprecedented sensitivity, spatial and spectral coverage of the integral fieldspectrograph MUSE at the Very Large Telescope. We developed a novel approachbased on the gas and stars kinematics to disentangle high-velocity gas in theoutflow from gas in the disc to spatially track the differences in their ISMproperties. This allowed us to reveal the presence of an ionisation structurewithin the extended outflows that can be interpreted with differentphotoionisation and shock conditions, and to trace tentative evidence ofoutflow-induced star formation (''positive'' feedback) in a galaxy of thesample, Centaurus A.

Interstellar medium properties and feedback in local AGN with the MAGNUM survey