Fig. 4.

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Radial structure of snapshot of set-up L3.85T27 for the full modelled region. Shown are the drift model, where ξ(Fo) = 0.1 (purple), and the PC model, where ξ(Fo) = 1.0 (orange). From the top left, the 12 panels show: (a) gas velocity ug, sound speed cs; (b) gas density ρg, dust density 104 × ρd (log); (c) drift velocity vD; (d) true degree of condensation of silicon and magnesium
; (e) net growth rate
, net decay rate
, and non-thermal sputtering
(log) times nd,FodV (where dV is the cell volume); (f) average grain radius rd; (g) Eddington factor fEdd; (h) extinction coefficient χH, Rosseland mean extinction coefficient χR; (i) gas temperature Tg, radiative temperature Tr, and dust temperature Td; (j) gas opacity κH and Rosseland mean opacity κR (log); (k) temperature ratios Td/Tr and (Tg/Tr)eq; and (l) dust-to-gas density ratio δdg. All properties are drawn vs the stellar radius R* (lower axis) and astronomical units (AU; upper axis). The grey horizontal lines are guides.
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