For Alpha Persei, the Pleiades, and Praesepe, the initial mass function is top-light (α_high ≈ 2.98 ± 0.22) and shows possible cluster-to-cluster scatter, based on Gaia DR3 plus N-body emulator inference.
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The initial conditions and initial mass functions of Alpha Persei, Pleiades and Praesepe
For Alpha Persei, the Pleiades, and Praesepe, the initial mass function is top-light (α_high ≈ 2.98 ± 0.22) and shows possible cluster-to-cluster scatter, based on Gaia DR3 plus N-body emulator inference.