Additional animations for Chapter 4:
Hydrodynamic Models of Tori

TOR 1	pressure in meridional plane in CGS units	pressure in equatorial plane in CGS units	density in meridional plane after shutting off energy and mass input	density in meridional plane for middle domain	density in equatorial plane for middle domain
TOR A	3D visualisation of an illuminated surface of constant density, temporal evolution	3D visualisation of an illuminated surface of constant density, rotating final state

Marc Schartmann

PhD Thesis: Models of Dust and Gas Tori in Active Galactic Nuclei

December 2006