Dust mass versus star formation rate for the Virgo SFDs (filled blue dots) compared to the KINGFISH spirals and dwarfs (small and large grey squares), and the DGS (red-purple triangles). The solid line shows the relation determined by da Cunha et al. (2010) for an IRAS selected sample of local star-forming galaxies. The orange shaded area stands for the dispersion of the relation. Evolution of the M_d − SFR relation for different amounts of dust mass destroyed by a single supernova event – M_cl = 100, 500, 1500  M_⊙ – is indicated by the dotted, dashed, dot-dashed lines, respectively (Hjorth et al. 2014).