Fig. 10
Metallicity a) and H2 depletion timescale b) as a function of specific SFR. Symbols are as in Fig. 9, but red points in a) indicate BCDs with higher gas fractions (MHI/ (MHI + M∗) > 0.5) BCDs. The dotted line in a) indicates solar metallicity, while the dashed line in b) shows the correlation found by Saintonge et al. (2011) for local star-forming disk galaxies of stellar masses M∗ ≳ 1010M⊙.
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