Protostellar Interferometric Line Survey of the Cygnus X region (PILS-Cygnus) - First results: Observations of CygX-N30

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Fig. 19

Relative abundances of each molecule relative to the column density of CH₃OH at each respective position. The white arrows represent upper limits, whereas the black bars represent the uncertainties (see Tables 5, 6 and 7).

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