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Fig. 11

image

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.

This figure is made of several images, please see below:

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