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Fig. 1

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Physical (approximately vertical) structure of d203-506. Upper panel: model profiles of gas density, gas temperature, and a−3.5 grain-size distribution, showing the highest and lowest dust temperatures (corresponding to amin and amax grain radii, respectively) as a function of depth into the PDR. The green curve shows the density of H2*(v4)${\rm{H}}_2^*\left( {v \ge 4} \right)$. Lower panels: abundance profiles of selected species. Bottom sketch: simplified sketch illustrating the PDR component of an externally irradiated protoplanetary disk. The different colored regions correspond to the chemical zones discussed in Sect. 4.

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