Fig. B.1.
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Scatter plot of stellar expansion rate, rc⋆/rc0⋆, versus the DM expansion rate, rcDM/r0DM, for the various types of isotropic velocity distributions analyzed in Figs. 4 and 5. The color code of the symbols and the labels are inherited from these two previous figures. The relationship is approximately a power law of exponent 0.85 (the solid red line). Two other exponents are shown for reference; in particular, 0.75 represents the scaling derived for circular orbits and given in Eq. (B.3).
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