Index

Chapter 2

Chapter 3

Chapter 4

Parameters of the hydrodynamic simulations

The following table gives an overview over the modified parameters within the simulations shown on this DVD. TOR 1 denotes our hydrodynamic standard model. Deviations from the parameters of the standard model are marked with red color.

model name mass loss rate
10-9Msun yr-1Msun-1		 supernova rate
10-10SNe yr-1Msun-1		 cooling initial condition stellar mass norm.const.
109 Msun		 planetary nebula mass
Msun
TOR 1 6.0 1.0 solar TTM 1.9 2.2
TOR 2 2.4 1.0 solar TTM 1.9 2.2
TOR 3 1.2 1.0 solar TTM 1.9 2.2
TOR 4 6.0 2.0 solar TTM 1.9 2.2
TOR 5 6.0 5.0 solar TTM 1.9 2.2
TOR 6 6.0 10.0 solar TTM 1.9 2.2
TOR 7 6.0 1.0 0.2 solar TTM 1.9 2.2
TOR 8 6.0 1.0 5.0 solar TTM 1.9 2.2
TOR 9 6.0 1.0 solar empty model space 1.9 2.2
TOR 10 6.0 1.0 solar cold initial condition, turbulent pressure 1.9 2.2
TOR 11 6.0 1.0 solar TTM 0.66 2.2
TOR A 12.0 1.0 solar TTM 0.66 2.2
TOR B 12.0 1.0 solar TTM 0.66 22.0
TOR C 2.4 1.0 solar TTM 0.66 2.2
TOR D 1.2 1.0 solar TTM 0.66 2.2
TOR E 6.0 0.5 solar TTM 1.9 2.2
TOR F 6.0 0.1 solar TTM 1.9 2.2
TOR G 6.0 0.01 solar TTM 1.9 2.2
TOR H 0.06 0.01 solar TTM 1.9 2.2

Marc Schartmann

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

December 2006