• DOI:10.1093/PASJ/PSV029
• Corpus ID: 118561826

Discovery of a nearby early-phase major cluster merger CIZA J1358.9-4750

@article{Kato2015DiscoveryOA,
  title={Discovery of a nearby early-phase major cluster merger CIZA J1358.9-4750},
  author={Y. Kato and Kazuhiro Nakazawa and Liyi Gu and Takuya Akahori and Motokazu Takizawa and Yutaka Fujita and K. Makishima},
  journal={arXiv: High Energy Astrophysical Phenomena},
  year={2015}
}

• Y. Kato, K. Nakazawa, +4 authors K. Makishima
• Published 9 April 2015
• Physics
• arXiv: High Energy Astrophysical Phenomena

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 position where the Suzaku-measured temperature exhibits a steep gradient. These properties indicate the presence of a shock discontinuity. The Mach number is estimated to be 1.32 from the temperature difference across the identified shock front, which gives the colliding velocity of approximately 1800 km/s. From optical redshifts of the member galaxies, the two clusters are indicated to be merging nearly on the sky plane. Thus, CIZA J1358.9-4750 is considered as a valuable nearby example of early-phase merger with a clear shock feature.