Fig. E.3
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Distribution of initial masses of stars in the core of R136, as found using BONNSAI. The dark blue solid line and the shaded area around it are the observed distribution and bootstrapped 2σ uncertainties. Red solid line is the best power law fit over the region 30–200M⊙ (light blue background), black dashed and dotted line represent 2σ uncertainty on the slope.
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