In astronomy, the intracluster medium is the superheated plasma that permeates a galaxy cluster. The gas consists mainly of ionized hydrogen and helium and accounts for most of the baryonic material i
The overlaid blue cloud illustrates the intracluster medium around the Spiderweb Galaxy, as seen when the universe was 3 billion years old.
Chandra image of the Perseus Cluster's radio lobes. These relativistic jets of plasma emit radio waves, are X-ray "cold", and appear as dark patches in stark contrast to the rest of the ICM.