Fig. 1
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Dust mass in SN ejecta as a function of the initial mass of nonrotating progenitor stars. Each panel corresponds to a different metallicity: [Fe/H] = 0 (top left), [Fe/H] = −1 (top right), [Fe/H] = −2 (bottom left), and [Fe/H] = −3 (bottom right). The solid, dotted, dashed, and dash-dotted lines represent no-rev, rev1, rev2, and rev3 models in each panel.
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