Max Planck Institute For Astrophysics 1

1. Centrally concentrated star formation in young clusters
2. Nucleosynthesis Conditions in Outflows of White Dwarfs Collapsing to Neutron 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
1