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Fig. 2


HIFI spectra of HO and HO (left) and HO (right) lines (in black) with continuum for NGC 6334I(N). The best-fit radiative transfer models are shown as red and blue lines over the spectra for constant parameters (Vinf = −0.7 and Vturb = 2.5 kms-1) and varying turbulent velocity. Vertical dotted lines indicate the VLSR. The spectra have been smoothed to 0.2 kms-1, and the continuum divided by a factor of two.

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