Fig. 8

Mass function slopes for all (individual) stars with mass ≥ 2 M⊙. Red filled circles are the present-day mass functions for the ejected stars (αej). Blue stars are the averaged present-day mass function slopes of the stars that remain in the clusters at 3 Myr (⟨ αin ⟩), while black open triangles are those at 0 Myr (i.e. IMF, ⟨ αi ⟩). The canonical value of the upper IMF, α2 = 2.3 (Eq. (1)), is indicated with a dotted grey line.
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