Discovery of a nearby early-phase major cluster merger CIZA J1358.9-4750
Yuichi Kato, Kazuhiro Nakazawa, Liyi Gu, Takuya Akahori, Motokazu, Takizawa, Yutaka Fujita, Kazuo Makishima

TL;DR
This paper reports the discovery and analysis of a nearby early-phase major galaxy cluster merger, CIZA J1358.9-4750, characterized by shock features and temperature gradients indicative of a recent collision.
Contribution
It provides detailed X-ray and optical evidence of an early-stage cluster merger with shock features, a rare nearby example for studying merger dynamics.
Findings
Identification of a shock front with Mach number 1.32
Detection of hot bridge region with temperature >9 keV
Clusters are merging nearly on the sky plane
Abstract
CIZA J1358.9-4750 is a nearby (z = 0.074) pair of clusters of galaxies located close to the Galactic plane. It consists of two X-Ray extended humps at north-west and south-east separated by 14 arcmin (~ 1.2 Mpc), and an X-Ray bright bridge-like structure in between. With Suzaku, the south-east hump was shown to have a temperature of 5.6 keV and the north-west one 4.6 keV. Neither humps exhibit significant central cool component. The bridge region has a temperature higher than 9 keV at the maximum, and this hot region is distributed almost orthogonal to the bridge axis in agreement with the shock heating seen in numerical simulations at an early phase of a head-on major merger. This resemblance is supported by good positional coincidence between the X-Ray peaks and cD galaxies associated with each cluster. In a short exposure XMM-Newton image, a significant intensity jump was found at a…
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Taxonomy
TopicsAstrophysical Phenomena and Observations · Galaxies: Formation, Evolution, Phenomena · Gamma-ray bursts and supernovae
