Visualisations of N-body simulations exploring stellar clusters, planetary systems, black hole dynamics, and multi-scale gravitational interactions.
How do debris disks evolve in star clusters?
Fractal: Substructured, sub-virial star-forming region hosting ~145 debris disks.
Plummer: Smooth, virialised cluster used as a comparison.
Do captured objects retain the encounters inclination? (Spoiler, the answer is no.)
How does the multi-scale, multi-physics algorithm Nemesis actually look in action?
Recoiling black holes can carry bound stellar populations, producing compact systems.