Fig. 6

Profiles of the inversion lines as computed for the best-fit models, which assume Rph = 3 × 1016 cm and the Tgas distribution from Crosas & Menten (1997), (blue dotted lines) are overplotted on the observed inversion transitions (solid lines) from Gong et al. (2015). Theoretical profiles for the same Tgas profile, but with the photodissociation radius reduced to Rph = 1.5 × 1016 cm are shown with red dashed lines. Vertical sticks show positions and relative intensities of hyperfine components.
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