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Fig. 10

image

Time evolution of the disk outer radius for different mass supply rates: 1 Myr-1 (dashed-line), 10 Myr-1 (dotted-line) and 100 Myr-1 (dashed-dotted line) under different assumptions regarding the gravitational field, that is, dominated by the central black-hole (black colour), by the CND (red colour) and by the host galaxy (blue colour).

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