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Fig. 6

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CS, HCN, CH3OH (sum of the 8 brightest lines at 252 GHz), and HNC lines observed with the IRAM 30-m telescope in comet C/2002 V1 (NEAT) on 16.5–17.6 February 2003. The spectra are plotted with the same horizontal scale to compare the line widths. The intensities of the spectra of HCN and HNC were divided by 10 and 2, respectively. Spectra are shifted vertically for clearer viewing.

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