Fig. 7.
Correlation between CO(1–0) luminosities and the total IR luminosity. The filled magenta squares are from T13 and filled turquoise circles are the sources from G10. The solid black line is the linear regression for MS galaxies (Sargent et al. 2014), and the dashed line is that for SBs (the regression lines are from the complete sample in Sargent et al. 2014).
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