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- W4283722706 abstract "Off-axis collisions between galaxy clusters may induce the phenomenon of sloshing, causing dense gas to be dragged from the cool core of a cluster, resulting in a spiral of enhanced X-ray emission. Abell 2199 displays signatures of sloshing in its core and it is possible that the orbital plane of the collision is seen nearly edge-on. We aim to evaluate whether the features of Abell 2199 can be explained by a sloshing spiral seen under a large inclination angle. To address this, we perform tailored hydrodynamical $N$-body simulations of a non-frontal collision with a galaxy group of $M_{200}=1.6times10^{13},{rm M_{odot}}$. We obtain a suitable scenario in which the group passed by the main cluster core 0.8 Gyr ago, with a pericentric separation of 292 kpc. Good agreement is obtained from the temperature maps as well as the residuals from a $beta$-model fit to the simulated X-ray emission. We find that under an inclination of $i=70^{circ}$ the simulation results remain consistent with the observations." @default.
- W4283722706 created "2022-07-01" @default.
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- W4283722706 date "2022-07-01" @default.
- W4283722706 modified "2023-10-15" @default.
- W4283722706 title "Simulating nearly edge-on sloshing in the galaxy cluster Abell 2199" @default.
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- W4283722706 doi "https://doi.org/10.1093/mnras/stac1829" @default.
- W4283722706 hasPublicationYear "2022" @default.
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