Fig. A.5.
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Observed lines of HNCO and HOCN at 3 mm with the IRAM 30 m radio telescope. The red line shows the synthetic spectra computed with the models described in Sect. 3. The column densities are the same as those derived from the lines observed in the Q-band. The bottom panels show the DNCO 404 − 303 and DCNO J = 2 − 1 lines. The derived line parameters are given in Table A.2.
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