Fig. 2

Panel a: median disc radius at the end of the simulation plotted against the average gas density within the cluster radius in the IM simulations. The colours and symbols correspond to the same process and number of stars as in Fig. 1. The lines connect the averages of the ten simulations with the same parameters. Panel b: same as in the left figure, but here we plot the median disc radius against the stellar density. The legend applies to both panels.
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