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Fig. 15.

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Cartoon summarizing the different regions (not drawn to scale) of Mrk 231 identified with the MRS observations and other literature results. Left: front view, that is, in the plane of the sky, where the molecular gas disk is seen close to face-on. Right: side view to emphasize the possible scenario to explain some of the observed non-circular motions in the ionized and warm molecular gas.

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