Fig. 5.
Left: total dust masses vs. diffuse X-ray plasma luminosities, both normalised by the stellar masses, for the galaxies observed with Chandra by Su et al. (2015). Right: SFRs vs. diffuse X-ray plasma luminosities. The symbols are as in Fig. 2, but the black stars in the right panel show robustly detected late-type galaxies (Mineo et al. 2012).
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