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. Author manuscript; available in PMC: 2016 Oct 7.
Published in final edited form as: Astron Astrophys. 2016 Sep 15;593:L12. doi: 10.1051/0004-6361/201628899

Fig. 2.

Fig. 2

Left: CO+ integrated emission (see Fig. 1). The pink-dashed line indicates the direction of the intensity cuts. The color circles indicate the positions where spectra were extracted. Right: Panel A to E show the intensity cuts (red continuum lines) of CO+, H13CO+, [CII], H2 and PAHs. In these panels, the gray continuum lines indicates the errors in the cuts. Panel F shows the comparison of the intensity cuts scaled to unity. In Panels A to F, the pink dot-dashed indicate the 3σ level for each species and the gray area indicates the position of the UC HII region. Panel G shows the CO+, [CII], H13CO+ and HCO+ spectra at IF, MP2 and PDR3. The color of the boxes are related to this positions (circles in left panel).