Clusters of Galaxies

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High-Resolution X-Ray Spectroscopic Constraints on Cooling-Flow Models for Clusters of Galaxies (2002, unknown): “…Peres et al. 1998; Allen 2000) and cluster cores have been shown conclusively to contain much lower X-ray temperature plasma than the ambient hot outer regions (Canizares et al. 1979, 1982; Mushotzky & Szymkowiak 1988), there is no consensus about how much mass has cooled from X-ray temperatures.”
Radio signature of cosmological structure formation shocks (2006, background): “Interestingly, the radio power of halos scales with the cluster X-ray luminosity (Feretti 2005) or, equivalently, with its temperature (Keshet et al. 2004).”