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Fig. 12

image

Influence of stellar evolution on the bound fraction as a function of initial cluster mass. The effect lessens with increasing mass, but is noticeable over the whole examined mass range. The differences are most likely due to the different re-virialization times after gas expulsion. The values for the clusters without stellar evolution are averaged over 3 simulations per mass, while one simulation per mass is used for those including stellar evolution.

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