Fig. 3

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Power-law slope of jtr versus rtr, , averaged for all the tracer particles within a single epoch, versus the final stellar mass (blue dots), as explained in the main text. The upper panel is for the scaling outside of RBH, the lower panel for the scaling inside RBH. The red lines show the median slope values aout = 0.82 (upper panel) and ain = 0.53 (lower panel, computed over masses ≥0.5 M⊙), and the shaded regions the rms value around the median.
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