Same as Figure 6, but for source 4C+19.71. Both mass outflow rates (bottom-left panel) and kinetic power (bottom-right panel) exhibit a clear enhancement near the radio core. The radial profiles show a sharp peak in both mass outflow rate and kinetic power at ∼15 kpc, spatially coincident with the radio core position (blue dashed line). Although the W₈₀ radial trend did not show a strong localized enhancement in the W₈₀ radial profile in Figure 11, the outflow rates and energetics maps confirm that substantial mass and energy are being injected near the AGN.