Page 2: Research news on Rich galaxy clusters

Rich galaxy clusters as a research area focus on the most massive, densely populated bound structures in the universe, typically hosting hundreds to thousands of galaxies embedded in a deep dark matter potential well and permeated by hot intracluster gas. Studies emphasize cluster mass assembly, baryon–dark matter distribution, intracluster medium thermodynamics, and galaxy evolution under extreme environmental effects such as ram-pressure stripping and tidal interactions. Rich clusters are also key cosmological probes, constraining structure formation, dark matter properties, and cosmological parameters through observations of their abundance, scaling relations, gravitational lensing, and X-ray and Sunyaev–Zel’dovich signatures.

Painting galaxy clusters by numbers (and physics)

Galaxy clusters are the most massive objects in the universe held together by gravity, containing up to several thousand individual galaxies and huge reservoirs of superheated, X-ray-emitting gas. The mass of this hot gas ...

Hubble snaps galaxy cluster's portrait

A massive, spacetime-warping cluster of galaxies is the setting of today's NASA/ESA Hubble Space Telescope image. The galaxy cluster in question is Abell 209, located 2.8 billion light-years away in the constellation Cetus ...

Phoenix galaxy cluster caught in the act of extreme cooling

The core of a massive cluster of galaxies appears to be pumping out far more stars than it should. Now researchers at MIT and elsewhere have discovered a key ingredient within the cluster that explains the core's prolific ...

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