Fueling the central engine of radio galaxies - II. The footprints of AGN feedback on the ISM of 3C 236

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Fig. 5

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Position–velocity diagram of the ¹²CO(2-1) emission along the major axis of the molecular gas disk of 3C 236 (dashed line in Fig. 4). Positions (Δx) are relative to the AGN. Velocities are relative to the CO . The contour levels are − 2σ, 2σ to 4.5σ in steps of 0.5σ, with σ = 3 mJy beam^-1 km s^-1.

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