Fig. 9.
Example of the evolution of three (out of seven solar-system equivalent systems) stars in one particular simulation for N = 2500 and rvir = 0.75 pc towards a high value of 𝒮eqiv. The coloured lines (green, orange and blue) each identify the evolution of one star in time. The vertical lines identify the moments when supernova are produced in the cluster; the thickness of these lines is proportional to the amount of mass that was injected in the supernova shell.
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