Fig. 5
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Time after which SF ends depending on the initial cluster mass. The empty circles are for the case that all stars above 8 M⊙ explode in a CCSN, the filled circles show the upper limit for the SF duration, for which it is assumed that only stars with masses <20 M⊙ explode in CCSNe. The plot is colour-coded for the metallicity, [Fe/H].
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