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Fig. 3.

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Schematic view of the outflow structure in a slice subtended by a solid angle ΔΩ and centered in a direction forming an angle θ with the MBH spin. This stratified structure comprises the AGN wind, the shocked wind (which extends up to a distance R(θ, t) from the MBH), the shocked ISM, and the unperturbed ISM. The illustration also shows the warped accretion disc that feeds the spinning MBH.

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