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Table 2.

Fraction of expanding clusters.

Ref. ages compilation ≤10 Myr (10; 30] Myr (30; 50] Myr > 50 Myr
Kharchenko et al. (2013) 17/32 (≃53%) 13/44 (≃30%) 4/14 (≃29%) 9/219 (≃4%)
Bossini et al. (2019) 6/18 (≃33%) 1/12 (≃8%) 2/93 (≃2%)
Cantat-Gaudin et al. (2020) 15/28 (≃54%) 43/108 (≃40%) 5/53 (≃9%) 14/320 (≃4%)
Dias et al. (2021) 21/41 (≃51%) 28/83 (≃34%) 4/43 (≃9%) 12/226 (≃5%)
Hunt & Reffert (2023) 34/51 (≃67%) 15/57 (≃26%) 1/39 (≃3%) 11/302 (≃4%)

Notes. The fraction and the absolute number of clusters that show significant expansion (at the 3σ level). Values are reported in four age bins, namely ≤10 Myr, between 10 − 30 Myr, between 30 − 50 Myr, and > 50 Myr, according to five different age compilations (left column). The only exception is the catalog of Bossini et al. (2019) for which we did not have any cluster younger than 10 Myr in common.

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