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Fig. 12

image

HIFI spectra of the H217O/H218O (left) and H216O (right) lines (in black), with continuum for G327.3–0.6 hot core pointed position. The best-fit model with varying (from line to line) and constant (2.6 km s-1) turbulent velocity is shown as a red and dashed blue line above the spectra. Vertical dotted lines indicate the VLSR (–43.2 km s-1 from the line modeling). The spectra have been smoothed to 0.2 km s-1, and the continuum is divided by a factor of two.

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