Fig. 12.
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Most massive young cluster mass vs. galaxy-wide SFR (Mcluster, max–Ṁ★) relation. The simulation data are color-coded by stage of the merger. The dashed red line represents the theoretical relation derived following Yan et al. (2017). The gray crosses represent observational data from Weidner & Kroupa (2004) and Schulz et al. (2015), which have a typical uncertainty of 0.3 dex.
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