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Fig. 8.

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Preferred model C of ESO 137−001. Upper panel: Hα is shown in color; X-ray in dark gray contours; CO in white contours; and stellar content in black contours. Lower panel: Hα velocity field. See Fig. 5 for the description of the contours and colors. The corresponding time evolution can be found online (observations_modelC.gif). The time evolution of the mass surface densities of the different gas phases can be found online (gasphases_modelC.gif).

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