Fig. 11
MH2/Mgas = MH2/(MHI+MH2) vs. sSFR (left panel) and vs. 12 + log(O/H) (right) for our sample and including data from the literature (Schruba et al. 2012; Bothwell et al. 2014); the left panel gives also the COLDGASS data (Huang & Kauffmann 2014). As in previous figures, the open triangles for Schruba et al. (2012) correspond to their compilation of data from the literature and the filled ones to their metal-poor dwarf observations.
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