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Fig. 9
Estimated disc inner radii (x-axis; Table 3) using relline (red) and relconv∗xillver (green) versus and the fitted break frequency from simultaneous RXTE observations (y-axis; Table 5). The dotted line represents the relation ν ∝ R− 3 / 2, which corresponds to the dynamical and viscous timescales for accretion onto a BH.
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