Astronomisches Rechen Institut 1

1. Evolution of star clusters with initial bulk rotation via N -body simulations
2. Milky Way globular clusters on cosmological timescales: I. Evolution of the orbital parameters in time-varying potentials
3. Milky Way globular clusters on cosmological timescales: II. Interaction with the Galactic centre
4. Milky Way globular clusters on cosmological timescales: III. Interaction rates
5. Statistical Analysis of the Probability of Interaction of Globular Clusters with Each Other and with the Galactic Center on the Cosmological Time Scale According to Gaia DR2 Data
6. The DRAGON-II simulations – I. Evolution of single and binary compact objects in star clusters with up to 1 million stars
7. 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
8. NGC 6240 supermassive black hole binary dynamical evolution based on Chandra data
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