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...

Täydet tiedot

Bibliografiset tiedot
Päätekijä: Binney, J
Aineistotyyppi: Journal article
Julkaistu: 2003

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