Results 281 to 284 of about 2,296,249 (284)

Turbulent heating in galaxy clusters brightest in X-rays

Nature, 2014
The hot (107 to 108 kelvin), X-ray-emitting intracluster medium (ICM) is the dominant baryonic constituent of clusters of galaxies. In the cores of many clusters, radiative energy losses from the ICM occur on timescales much shorter than the age of the ...
I. Zhuravleva, E. Churazov, A. Schekochihin, Steven W. Allen, Steven W. Allen, P. Arévalo, P. Arévalo, A. C. Fabian, W. Forman, J. Sanders, A. Simionescu, R. Sunyaev, A. Vikhlinin, Norbert Werner   +13 more
semanticscholar   +1 more source

Galaxy Clusters

The Dark Energy Survey, 2020
T. Jeltema, Tim McKay, Chris Miller, Joe Mohr, Kathy Romer   +4 more
semanticscholar   +1 more source

GALAXY CLUSTERS:

More Things in the Heavens, 2019

semanticscholar   +1 more source