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Table 6.

Initial and current (final) masses of the runaway star and progenitor for different cluster ages.

log(age[yr]) Mini − run Mini − pro Mrun Mpro
6.6 46 ± 1 & 54 64 41 & 32 21
6.7 35 42 32 16
6.8 28 31 26 20

Notes. The masses are given in solar masses.

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