High-velocity, |v_proj| > 200 km s⁻¹, CO(2–1) outflow emission measured in the annulus sectors presented in Figs. 5 and 6. The top and bottom panels correspond to the blue- and red-shifted emissions of the outflow, respectively. The x-axis velocities and the distance to the nucleus indicated in each panel are deprojected values assuming a perpendicular to the disk outflow and a galaxy inclination, i, of 43° (Pereira-Santaella et al. 2016). The dotted vertical line traces the expected velocity of a cloud in the gravitational potential at each distance with an initial v ∼ 600 km s⁻¹ at 190 pc. The horizontal dashed line indicates the average 1σ noise of the spectra per channel.