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

Writer's picture: Asif Iqbal AhangarAsif Iqbal Ahangar

Updated: Feb 4, 2024








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.







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