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Fig. 4

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HC3N, CS, HCN, CH3OH (sum of the 3 brightest lines at 157 GHz) and HNC lines observed with the IRAM 30-m telescope in comet C/2002 X5 (Kudo-Fujikawa) on 26.5 January 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 12.5 and 2.5, respectively. Spectra are shifted vertically for clearer viewing.

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