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We present multimolecular line maps obtained with the Mopra telescope towards the southern giant molecular cloud (GMC) complex G333, associated with the H  ii  region RCW 106. We have characterized the GMC by decomposing the 3D data cubes with  gaussclumps , and investigated spatial correlations among different molecules with principal component analysis (PCA). We find no correlation between clump size and linewidth, but a strong correlation between emission luminosity and linewidth. PCA classifies molecules into high‐ and low‐density tracers, and reveals that HCO +  and N 2 H +  are anticorrelated.

Molecular line mapping of the giant molecular cloud associated with RCW 106 – III. Multimolecular line mapping