Unraveling the Mysteries of AGN Heating: Exploring Models in Galaxy Clusters

Fig. 1 Evolution of temperature profiles of the ICM with Efferversent heating with two different values of mechanical energy injected by bouyont radio bubbles as they move upwards in the ICM

Fig. 2 Evolution of temperature profiles of the ICM with acoustic heating with two different values of mechanical energy injected by sound waves as they pass through ICM

Fig. 3 Relation between average injected luminosity and the cluster mass for the effervesent and acoustic heating.