Reproduzindo o estado dissociativo do aglomerado de galáxias Abell 56 por meio de simulações hidrodinâmicas

Abstract

In galaxy cluster collisions, the gas can be separated from dark matter halos. Abell 56 displays signatures of a dissociative bullet-like merger with a possible high inclination angle between the plane of orbit and the sky. Our objective is to provide a comprehensive description of the features observed in the collision scenario of Abell 56. Additionally, we aim to apply a potential weak lensing mass bias correction attributed to the merger to evaluate its impact on our findings. To investigate this, we perform tailored hydrodynamical 𝑁-body simulations, varying the impact parameter. We initially identified an early scenario at 0.12 Gyr after the central passage that reproduces some observational features. However, the mean temperature of 9.7 keV exceeded the observed value. Our best model corresponds to the late scenario at 0.52 Gyr after the pericenter, reproducing observed features of Abell 56, with an inclination of 58◦. These features include the offset of 103 kpc between the main gas density peak and the south dark matter density peak, gas morphology, a line of sight relative velocity of 184 km s−1, and a mean temperature of 6.7 keV. This late model provides a plausible scenario to describe the dynamics of Abell 56. The weak lensing mass bias did not significantly impact the overall dynamics of this cluster merger.