clumpy | i=0° | i=30° | i=60° | i=90° | homogeneous | i=0° | i=30° | i=60° | i=90° |
---|
clumpy | i=0° | i=30° | i=60° | i=90° |
---|---|---|---|---|
homogeneous | i=0° | i=30° | i=60° | i=90° |
Marc Schartmann |
PhD Thesis: Models of Dust and Gas Tori in Active Galactic Nuclei |
December 2006 |