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

Open Access

Fig. 19

Distribution of the logarithm of mass for OCs with an age under 50 Myr and simulated distribution of masses using different ICMFs: Trujillo-Gomez et al. (2019), Trujillo-Gomez et al. (2019) with M_min ~ 500 M_⊙ and M_max ~ 1000 M_⊙, and the adopted ICMF (skewed lognormal with α = 2, location = 2.3, and scale = 0.5).

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