Fig. 9.
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Top panel: star formation rate as a function of stellar mass for LSB-D (marked by the red circle, and for a sample of galaxies in the Local Universe. LITTLE-THINGS (Oh et al. 2015; Iorio et al. 2017) and THINGS galaxies are marked by orange and blue triangles. Local low surface brightness galaxies (LSBGs) from McGaugh (2011, 2017) are in green. The dashed line shows a linear relation fitted betwee the LSBGs and THINGS samples. Central panel: specific star formation rate as a function of stellar mass for the same sample as in the top panel. The dashed-dotted line marks the inverse Hubble time, i.e. galaxies on the relation reach their current stellar mass with their average SFR since the Big Bang. Bottom panel: depletion time as a function of stellar mass for LSB-D and the samples of galaxies in the Local Universe. The dashed line marks the linear fit relation for the Local LSBGs sample.
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