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Super-massive black holes (SMBH) are present at the center of most galaxies,with the related mass accretion processes giving origin to outflows in ActiveGalactic Nuclei (AGN). It has been presumed that only intense winds fromluminous AGN were able to suppress star formation until the discovery of a newclass of galaxies with no recent star formation and with the nucleus in aquiescent state showing kpc scale outflows. We used SDSS MaNGA and GeminiIntegral Field Spectroscopy of the prototype Red Geyser Akira and found thatthe orientation of the outflow changes by about 50$^\circ$ from its nucleus tokpc scales. A possible interpretation is that the outflow is produced by aprecessing accretion disk due to a misalignment between the orientation of thedisk and the spin of the SMBH. The precession of the central source is alsosupported by a similar change in the orientation of the ionization pattern.Although similar behavior has commonly being reported for collimatedrelativistic jets, the precession of an AGN wide wind is reported here for thefirst time, implying on a larger work surface of the wind, which in turnincreases the star formation suppression efficiency of the outflow.

Precessing winds from the nucleus of the prototype Red Geyser?