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Fig. 1.

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Lines of HCCNCH+ observed toward TMC-1. The J = 4–3 and J = 5–4 lines were observed with the Yebes 40 m telescope and the J = 9–8 and J = 10–9 lines with the IRAM 30 m telescope. Unidentified lines are labeled as “U”. The red lines correspond to the line profiles calculated with the LVG method adopting a column density for HCCNCH+ of 3.0 × 1010 cm−2, a kinetic temperature of 10 K, a volume density of H2 of 4 × 104 cm3, a linewidth of 0.60 km s−1, and an emission size of 40″ in radius (see text).

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