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The BIG X-ray tail
Chong Ge, Ming Sun, Masafumi Yagi +9
Galaxy clusters grow primarily through the continuous accretion of group-scale haloes. Group galaxies experience preprocessing during their journey into clusters. A star-bursting c…
Constraining black hole feedback in galaxy clusters from X-ray power spectra
Annie Heinrich, Yi-Hao Chen, Sebastian Heinz +2
Jets launched by the supermassive black holes in the centers of cool-core clusters are the most likely heat source to solve the cooling flow problem. One way for this heating to oc…
Evolution of Splashback Boundaries and Gaseous Outskirts: Insights from Mergers of Self-similar Galaxy Clusters
Congyao Zhang, Irina Zhuravleva, Andrey Kravtsov +1
A self-similar spherical collapse model predicts a dark matter (DM) splashback and accretion shock in the outskirts of galaxy clusters while misses a key ingredient of structure fo…