Fig. 7
Comparison of the observed spectra with the results of our best-fit models for the
two different physical profiles. The observed line emission is shown as black
histograms in each spectrum. The red, green, and blue lines show the best-fit
results of the Rolffs model, the Nomura model with all spectra, and the Nomura model
excluding the HDO spectrum at 893 GHz (X
;
X
).
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