Fraction of dust mass (M_dust, blue line) and stellar mass (M_★, orange line) enclosed within a sphere of radius r. Total masses are indicated in the legend. Vertical dashed lines mark the radii containing 90% of the total mass for each component (r_dust,90 and r_*,90) with values reported in the figure. As a reference, we show the enclosed dust for the S20 model in the homogeneous ($r_{\text{dust, }90}^{\text{S}20\text{\hspace{0.17em}hom}}\simeq 90$, green line) and radiation– pressure ($M_{\text{dust }}^{\text{S}20\text{\hspace{0.17em}RP}}$, magenta line) case, as well as the radii enclosing the 90% of the total mass in both cases ($r_{\text{dust,90 }}^{S20\text{\hspace{0.17em}hom}}$ and $r_{\text{dust,90 }}^{\text{S}20\text{\hspace{0.17em}RP}}$, respectively).