Fig. A.3.
Observed lines of HC7N with the Yebes 40 m telescope. The rotational quantum numbers are indicated in the top-left side of each panel. The same transitions for the ν15 state are shown in the middle (e component) and right panels (f component). The intensity scale is antenna temperature in mK. The abscissa corresponds to LSR velocities in km s−1. The vertical red dotted line at −26.5 km s−1 indicates the systemic velocity of the envelope (Cernicharo et al. 2000, 2018).
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