Heating of the cooling flow The feedback effervescent heating model

  • Nasser Mohamed Ahmed
  • Published 2008
The standard cooling flow model has predicted a large amount o f a c ol gas in the clusters of galaxies. The failure of the Cha ndr and XXM-Newton telescopes to detect a cooling gas (below 1-2 keV ) in the clusters of galaxies has suggested that some heating process must work to suppress the cooling. The most likely heating so urce is the heating by AGNs… (More)