Fig. B.1

Spectrum of the C2H N = 1–0 line. The different hyperfine components are indicated with their relative intensities for the SW (top) and NE (bottom) absorptions. Note the clear detection of the two strongest hyperfine components arising from FG0.89NE. The red curve shows the LTE synthetic spectrum, taking column densities of 1.3 × 1015 and 4 × 1013 cm-2 toward the SW and NE images respectively, and a rotation temperature of 5.14 K.
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