Fig. 4

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Cumulative distribution of the cluster meteor masses. The dashed red line represents a linear part of the plot, which is fitted with a line of slope k = −1.10 and which was used for the calculation of the mass distribution index. The dashed green line fits masses between 0.02 g and 0.08 g. These limits, used to calculate the total mass of the cluster, are marked by vertical dashed blue lines. The slope of this line is k = −0.49.
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