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Fig. 7.

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Light curves for the ionising continuum from the central source and for the red and blue BEL wings. The x axis represents time in units of the orbital period, while the y axis represents the normalised flux. Upper panel: Binary scenario with M1 = 107 M and M2 = 106 M. The separation is a = 10−3.9 pc. Lower panel: Single MBH scenario with the same ionising continuum as in the binary case.

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