| |
 |
| Paper: |
Emission-line Outflows — the Evidence for AGN-induced Feedback |
| Volume: |
373, The Central Engine of Active Galactic Nuclei |
| Page: |
347 |
| Authors: |
Holt, J.; Tadhunter, C.N.; Morganti, R. |
| Abstract: |
We present a brief summary of a detailed optical, radio and infrared study of the young radio source PKS 1549–79 in which the obscured black hole is growing rapidly. We detect a fast outflow in the emission-line gas, although currently these are less powerful than required by galaxy evolution models that incorporate AGN feedback. PKS 1549–79 is an important source as it links a number of different types of AGN (quasar, radio galaxy, NLS1, ULIRG) and is a rapidly evolving galaxy in the local universe. See Holt et al. (2006) for further details. |
|
|
|
|
|
