Concentration of various condensates (normalized to hydrogen atom number density) as a function of radius and temperature from our calculation using the thermo-chemical equilibrium code GGCHEM (Woitke et al. 2018). Top: plot showing the concentration using the photospheric elemental abundances of HD 144432. Bottom: plot showing the concentration using Solar elemental abundances. For clarity, we show a selection of the condensates: we plot only those species which are among the top three most abundant condensates for at least one temperature value. The T (r) relation follows our best-fit TGMdust model with iron grains. The gas pressure-temperature profile follows a power law with p = 3.16 × 10⁻² bar at the maximum temperature T = 2000 K, and p = 1.79 × 10⁻⁶ bar at the minimum temperature T = 277.5 K.