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Fig. 11


Effect of stellar evolution. Covering the first 9.5 Myr (respectively 8.9 Myr after the beginning of gas expulsion) for two 5 × 103M clusters. While the reversion process after gas expulsion is ongoing for the cluster without stellar evolution (left panel), the first SN disturb the process of re-virialization in the more realistic scenario including stellar evolution (right panel). The effect is more distinct in these lower mass clusters.

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