Fig. 2.
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Fraction of all stars located in their parent cluster for the galaxy-wide ECMF of Eq. (4) and for a single starburst. Clusters orbit the galaxy at Rg = 4 kpc, Rg = 8 kpc, and Rg = 12 kpc (different thickness of solid lines). These clusters have the Solar metallicity of Z = 0.014. Models of Z = 0.006 and Z = 0.002 for Rg = 8 kpc are shown by the dashed and dotted lines.
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