Giersz M 1

1. Evolution of star clusters with initial bulk rotation via N -body simulations
2. The DRAGON-II simulations – I. Evolution of single and binary compact objects in star clusters with up to 1 million stars
3. The DRAGON-II simulations – III. Compact binary mergers in clusters with up to 1 million stars: mass, spin, eccentricity, merger rate, and pair instability supernovae rate
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