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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. 15.

Fig. 15

Grid of LVG excitation and radiative transfer models for CH3CN, H2CO, CH3OH, and HC3N lines towards the PDR position assuming uniform beam filling and using column densities shown in Table 3. The best fits are those with the higher rmsmin / rms value.