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. Author manuscript; available in PMC: 2017 Nov 13.
Published in final edited form as: Astron Astrophys. 2017 Jul;603:A124. doi: 10.1051/0004-6361/201730459

Fig. 21.

Fig. 21

Isobaric PDR model for the Orion Bar with Pth/k = 108 K cm−3 and χ = 2 × 104. The thick horizontal bars show the inferred abundances of HCO, H2CO, and CH3OH towards the PDR edge. In this model, these molecules are formed only through gas-phase reactions.