Cooling Flows or Heating Flows?
It is now clear that AGN heat cooling flows, largely by driving winds. The winds may contain a relativistic component that generates powerful synchrotron radiation, but it is not clear that all winds do so. The spatial and temporal stability of the AGN/cooling flow interaction are discussed. Collima...
| Egile nagusia: | |
|---|---|
| Formatua: | Journal article |
| Argitaratua: |
2003
|