Fig. 4.

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Relationship between g1 and the slope of the post-collision mass function, αpc (for stars in the mass range 0.2–0.8 M⊙), for various shapes of the IMF, namely for various values of the slope in the intermediate-mass range, α1, and for various values of fext. In all models, the values of α0 and α2 are fixed to −0.3 and −2.3, respectively. The models are compared to the (N(G1)/N(tot)) − αpd found in the observations.
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