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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. 4.

Fig. 4

Example of ortho- and para-H213CO lines (black histogram spectra). A non-LTE LVG model (Tk ≃ 200 K, n(H2) ≃ 1 × 106 cm−3, N(o-H213CO)=7.3×1011cm-2, and N(p-H213CO)=2.3×1011cm-2) is shown overlaid in red (see Sect. 5.2).