Fig. 16
Mass function of the Her-Lyr association compared to the initial mass function (IMF). Only good candidates (membership criterion + and ? in Table 11) are included. The number of stars is N = μM− α with the stellar mass M in M⊙, the proportionality factor μ, and the index α (see text). Only stars with M ≥ 0.8 M⊙ are used to fit μ. See text for further explanations.
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