activity
20182021
most citedTurbulence decay in the density-stratified intracluster medium

18 citations · 36 across the 2 of their papers we have counts for

collaborators

9 papers

astro-ph.CO2021

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…

astro-ph.HE2020

Pairs of Giant Shock Waves (N-Waves) in Merging Galaxy Clusters

Congyao Zhang, Eugene Churazov, Irina Zhuravleva

When a subcluster merges with a larger galaxy cluster, a bow shock is driven ahead of the subcluster. At a later merger stage, this bow shock separates from the subcluster, becomin…

astro-ph.HE202018 cited

Collision of Merger and Accretion Shocks: Formation of Mpc-scale Contact Discontinuity in the Perseus Cluster

Congyao Zhang, Eugene Churazov, Klaus Dolag +2

Two Mpc-size contact discontinuities have recently been identified in the XMM-Newton and Suzaku X-ray observations of the outskirts of the Perseus cluster (Walker et al. 2020). The…

astro-ph.GA2020

Encounters of Merger and Accretion Shocks in Galaxy Clusters and their Effects on Intracluster Medium

Congyao Zhang, Eugene Churazov, Klaus Dolag +2

Several types/classes of shocks naturally arise during formation and evolution of galaxy clusters. One such class is represented by accretion shocks, associated with deceleration o…

astro-ph.GA2019

Runaway Merger Shocks in Galaxy Cluster Outskirts and Radio Relics

Congyao Zhang, Eugene Churazov, William R. Forman +1

Moderately strong shocks arise naturally when two subclusters merge. For instance, when a smaller subcluster falls into the gravitational potential of a more massive cluster, a bow…

astro-ph.CO201918 cited

Turbulence decay in the density-stratified intracluster medium

Xun Shi, Congyao Zhang

Turbulence evolution in a density-stratified medium differs from that of homogeneous isotropic turbulence described by the Kolmogorov picture. We evaluate the degree of this effect…