Here you can find some cool animations of my hydrodynamical simulations. What you can see is a turbulent molecular cloud falling into binaries of super-massive black holes. The different videos are a combination of 2 things: 1) the relative inclinations between the binary and cloud orbits, and 2) the distance the cloud is passing from the binary center of mass.
- Aligned orbits, three impact parameters:
- Counter-aligned orbits, three impact parameters:
- Perpendicular orbits (edge-on), three impact parameters:
- Perpendicular orbits (face-on), three impact parameters: