Fig. 2.
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Selected lines of the isomer 3-CNACY observed in the K and Q bands. The abscissa is the rest frequency in MHz adopting a VLSR for the source of 5.83 km s−1 (Cernicharo et al. 2020). The ordinate is the antenna temperature corrected for atmospheric losses in mK (same scale for all panels). The labels α, β, and γ correspond to unresolved doublets with Ka = 0,1, Ka = 1,2, and Ka = 2,3, respectively. The red line corresponds to the synthetic spectrum computed with the physical parameters discussed in the text.
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