Fig. 4.

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Cliffhanger region for different MBH masses in the (1 − e, a) plane, where a is shown through its ratio with the influence radius. The darker regions are partly covered by lighter regions as all the regions extend up to the upper axis. All regions share a similar triangular shape, which is pushed towards the upper left corner of the plot as M• increases, effectively shrinking the available cliffhanger region for a < Rinf. For M• = 107 M⊙ the whole cliffhanger region is located outside the a = Rinf line.
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