The XRISM collaboration has discovered flows of hot gas in the core of the Centaurus Cluster. By comparing state-of-the-art X ...

Scientists used XRISM to detect hot gas flows in Centaurus Cluster, proving that galaxy collisions cause gas movement and ...

Scientists have finally solved a long-standing mystery: why do galaxy clusters stay hot? Thanks to a new discovery from the ...

This is the first direct evidence for this kind of “sloshing”, validating a long-hypothesized picture of the evolution of the universe. It also solves a long-standing unsolved mystery for ...

Intergalactic “sloshing” of hot gas. Collisions between clusters generate a “sloshing” effect for the intracluster medium, causing vast flows of gas that cause the content of the clusters to oscillate ...