Volume filling factor (top panels) and the associated mass fraction (bottom panels) in each temperature range above the disc on both sides (|z| > 200pc) for the models with: SB wind only (C.MHD.100SF, left) and with SB + AGN wind (C.MHD.100SF.360°.L2, right) shown in five different times: t = 0.0, 0.525, 1.05, 1.575, and 2.1 Myr. The model with AGN wind removes a bigger fraction of cold and warm gas (right panels), specially after 2.1 Myr of evolution, when the AGN-wind remnant is no longer visible. This suggests that, at least at the scales studied here (< 1 kpc), the past AGN-wind activity is a determining factor in the production of cold outflows, that are the most massive component of the gas being ejected.