Fig. 3
Dependence of the warm dust mass Mwd of the sample of ~1000 SDSS compact galaxies with reliably derived oxygen abundance on a) total galaxy stellar mass M∗ and b) mass of the young stellar population My. Red and blue filled circles are for galaxies with EW(Hβ) ≥ 50 Å and EW(Hβ) < 50 Å, respectively. In both panels, solid lines are fits to the data where Mwd is calculated adopting β = 2.
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