Fig. B.2
SFE as a function of morphological type for the WISE-selected subsample of 89 galaxies with both high-quality WISE and CO data. The color coding is as in Fig. 1. Filled circles denote galaxies belonging to the IRTZ (lower panel). The lines show the mean value (full line) and dispersion (dashed lines) found by Bigiel et al. (2011) for a sample of spiral and starburst galaxies.
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