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Fig. 1.

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Lines of NC4NH+ observed toward TMC-1. Blanked channels correspond to negative artifacts resulting from the frequency switching observing mode. Unidentified lines are labeled as U. The red lines correspond to the line profiles calculated under LTE adopting a column density of 1.2 × 1010 cm−2, a rotational temperature of 5.6 K, a line width of 0.60 km s−1, and an emission size of 40″ in radius (see text).

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