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Fig. 3.
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Accretion rates onto the isolated BHs orbiting the SMBH in units of their Eddington rate (see Eq. (13)) as a function of their distance from the center of the galaxy. Both axes are on a logarithmic scale. We plot the three regimes of SMBH accretion (ζ1 − ζ3 from bottom to top).
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