Simulations of the merging galaxy cluster Abell 2034: what determines the level of separation between gas and dark matter
Micheli T. Moura, Rubens E. G. Machado, Rog\'erio Monteiro-Oliveira

TL;DR
This study uses hydrodynamical simulations to understand the factors influencing gas-dark matter separation in the merging galaxy cluster Abell 2034, revealing the importance of central gas density ratios.
Contribution
The paper introduces a detailed simulation-based analysis of Abell 2034, highlighting the role of gas density ratios in dissociation during cluster mergers.
Findings
Gas density ratios significantly affect dissociation levels.
Simulation reproduces observed X-ray and DM features.
Impact parameter and viewing angle are crucial for accurate modeling.
Abstract
Cluster mergers are an important laboratory for studying the behaviour of dark matter (DM) and intracluster gas. There are dissociative collisions that can separate the intracluster gas from the DM. Abell 2034 presents clear dissociative features observed by X-rays and gravitational lensing. The cluster, at = 0.114, consists of two substructures with mass ratio of about 1:2.2, separated by 720 kpc. The X-ray emission peak is offcentred from the south DM peak by 350 kpc. Using N-body hydrodynamical simulations, we aim to reconstruct the dynamic history of the collision, reproducing the observed features, and also to explore the conditions that led to the dissociation. Our best model assuming that the collision is close to the plane of the sky, with a small impact parameter, observed 0.26 Gyr after central passage, reproduces the observed features of this cluster, such as…
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