Open cluster dissolution rate and the initial cluster mass function in the solar neighbourhood - Modelling the age and mass distributions of clusters observed by Gaia

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Fig. 1

Distribution of King radii for 1724 OCs (in light blue). The dark blue histogram represents the distribution of King radii excluding clusters with poor quality fits (classified as R4; see Sect. 4.1.1). Bin widths were set using Knuth’s rule (Knuth 2006).

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