Simulating nearly edge-on sloshing in the galaxy cluster Abell 2199

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