Fig. 2.

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Complementary cumulative distribution function (CCDF) plot and the linear fitting of the synthesized CMFs (in cyan) for W43-MM1 by setting fb = 1 and ϵcore = 0.2. (a)–(c) The cases of mmax = 150 M⊙, half the original number of stars (Nstar/2) and twice the original number of stars (Nstar * 2), respectively; (d) The case in which ϵcore decreases with decreasing core mass. ϵcore was randomly selected from the range (0.2, 0.4); (e) The case in which ϵcore increases with decreasing core mass. ϵcore was randomly selected from the range (0.2, 0.4); (f) Same as panel e, but ϵcore is in the range (0.1, 0.3). All selected ϵcore in panels d, e, and f are sorted in descending or ascending order. All CCDFs (both observed and synthesized) were normalized to 1 at the mass completeness level marked by the left vertical dashed line.
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