Abell 3571 is a nearby, X-ray-bright galaxy cluster located in the Shapley Supercluster. Although it appears morphologically relaxed in X-ray images, multiwavelength observations reveal subtle indications of residual dynamical activity likely associated with past merger events. Using wide-field (1^ ̧irc 1^ ̧irc) data from the Einstein Probe Follow-up X-ray Telescope (), we extended measurements of the cluster’s properties beyond its R₅00 radius. We detect surface-brightness excesses on both the northern and southern sides, consistent with previous results. The temperature, pressure, and entropy in the northern excess region are lower than the average values, whereas those on the southern side are slightly higher. However, we find no evidence of cold fronts or shocks. These features can be interpreted as sloshing motions triggered by an off-center minor merger. Our findings suggest that, despite its symmetric appearance, A3571 is still recovering from a minor merger and is currently in a post-merger phase. This work also demonstrates the excellent capability of for probing the outskirts of galaxy clusters. EP-FXT XMM-Newton EP-FXT
Zheng et al. (Wed,) studied this question.