Fig. 4
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Other molecules detected in the direction of AFGL 2298. Molecules and transitions are indicated inside each spectrum. We note that different velocity ranges are depicted, and that the temperature scale is kept the same for each row. In the case of molecules with hyperfine splitting, the positions and relative intensities are indicated by the red lines below (above) the spectrum, for velocities of 36 (46) km s−1.
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