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...
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| Формат: | Journal article |
| Опубликовано: |
2003
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