Fig. 6
Line profiles of the [C ii], [O i], CO 16−15, CO 2−1, C18O 1−0, and 13CO 1−0 lines at the position of the [O i] peak (0, 20 close to IRS 2), at IRS 1 (0, 0), and at the interface (−40, −54). The lines are averaged in a Gaussian beam of 17.3′′ FWHM (telescope + convolution kernel) except for the 13CO and C18O lines that can only be treated at the lower resolution of 23′′.
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