Linked from

The 19 pages that link to Intracluster medium, each with the reason it gives.

• Ram-pressure strippingRelated: Its density supplies the gas that generates stripping pressure.

• Virgo ClusterRelated: Its X-ray-emitting gas is a major component of Virgo’s baryonic matter.

• Chandra X-ray ObservatoryRelated: Chandra’s observations measure this X-ray-bright gas and reveal how clusters gain and lose energy.

• Radio galaxyRelated: Radio lobes expand into this gas and can create cavities and shocks.

• Sunyaev–Zel'dovich effectRelated: Its free electrons scatter the background radiation throughout a cluster.

• Bullet ClusterRelated: Collisions make this gas interact and slow, leaving it displaced from the lensing mass.

• Shapley SuperclusterRelated: Its X-ray emission helps astronomers identify and characterize clusters in the region.

• Cygnus ARelated: Cygnus A’s lobes displace this gas and leave observable cavities.

• Abell 1689Related: This X-ray-emitting gas is a major component of the cluster’s ordinary matter.

• NGC 1275Related: NGC 1275 injects energy into the Perseus Cluster’s central intracluster medium.

• cD galaxyRelated: Its gravitational and thermal environment affects the growth and surroundings of central cD galaxies.