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The growing evidence for energy-conserving outflows in powerful and luminousAGN supports the idea that high-velocity winds launched from the accretion discevolve systematically after undergoing a shock with the ambient medium and thatthey are capable to expel enough mass and energy so as to produce feedback.This talk will give an overview of recent results on AGN ultra fast outflows,with focus on grating X-ray spectra of bright sources. I will review how UFOwork, their observational properties and their relation with AGN outflows inother bands, what is their impact on the host galaxies and their role infeedback processes.

Ultra fast outflows, and their connection to accretion and ejection processes in AGNs