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Fig. 16


Comparison between removing and keeping escaped stars in the calculations. Removing escapers from clusters situated in a tidal field at the solar distance does not seem to have a significant impact on the bound fraction over the considered mass range. The overlap with the comparison plot including the escapers in the total cluster mass is notable in wide parts. For the clusters with removed stars, one simulation per mass is used, while the data points for the clusters keeping escapers consider 2 runs per mass.

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