Fig. 14.
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A) Specific angular momentum, Lz, as a function of the cylindrical radius, R, during the orbital migration of the BH. The large sky-blue arrows indicate the flow of time, t. The orange solid lines trace the expected values for the model galaxy. The curve in blue (red) shows the coordinates before (after) Lz has reached a maximum. The black lines indicate evolution at a constant Lz. The circles numbered 1 and 2 single out specific phases of evolution. B) Run of azimuthal velocity, vϕ, against radius, R. The axes have been shifted for clarity. The colour-coding for the other curves and symbols is as for (A).
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