Overmassive and Undermassive Massive Black Holes: The Role of Environment and Gravitational-Wave Recoils

Open Access

Fig. 6.

Redshift evolution of the median M_BH/M_* ratio for a model in which no GW kicks and ejections are included. The upper (lower) panel corresponds to galaxies with M_* > 10⁸ M_⊙ (M_* > 10¹⁰ M_⊙) and solid lines correspond to the model without (with) ejections after gravitational recoils. The colour coding and mass dependence are the same as in the upper panel of Fig. 2.

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