THE HYDRODYNAMIC EFFECTS OF NUCLEAR ACTIVE GALAXY WINDS ON HOST GALAXIES.
In order to test the hypothesized existence of a powerful, thermal wind in active galactic nuclei, the hydrodynamic effects of such a wind on a model galactic interstellar medium (ISM) are investigated. The properties of several model ISMs are derived from observations of the Milky Way's ISM an...
| Main Author: | |
|---|---|
| Other Authors: | |
| Language: | en |
| Published: |
The University of Arizona.
1984
|
| Subjects: | |
| Online Access: | http://hdl.handle.net/10150/187865 |