Fig. 10
In black: 
O lines
observed with HIFI. In red: best-fit model obtained when adding an absorbing layer
with a O
column density of 1 × 1012 cm-2. The inner abundance is
1 × 10-8 and the outer abundance is 3 × 10-11. The detected
line at a velocity of 15 km s-1 in the panel of the 489 GHz transition is
CH3OH at 489.0368 GHz. Also, the line observed at a velocity of
−10 km s-1 in the panel of the 970 GHz transition is p-H2O
at 970.3152 GHz.
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