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Fig. 7

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Plot showing the effect of increasing electron fractional abundance (thick black curves, calculated using a constant kinetic temperature of 12 K) and kinetic temperature (dashed curves, calculated using a negligible electron abundance) on the 4  →  3/1  →  0 line intensity ratios of H13CO+ and HN13C, for gas with an H2 density of 6 × 105 cm-3 and H13CO+ and HN13C column densities of 8.8 × 1011 cm-2 and 5.1 × 1011 cm-2 respectively. The grey bar shows the observed H13CO+ 4  →  3/1  →  0 line intensity ratio towards NGC 1333, taking into account the 1σ errors in the observations. The thin black line shows the upper limit to the observed HN13C 4  →  3/1  →  0 line intensity ratio towards NGC 1333.

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