CLASH星团A209的弱合并情景

Wencheng Feng, Heng Yu, Haihui Zhao, Xiaolan Hou, Shumei Jia, Chengkui Li, Yulin Cheng, Paolo Tozzi, Ming Sun, Yong chen
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摘要

我们根据钱德拉和 XMM-Newton 观测数据研究了 Abell 209 的结构和动力学特性。我们利用等高线分档法获得了详细的温度、压力和熵图,并发现了一个位于西北方向的热区。X 射线亮度残差图和相应的温度曲线揭示了西北方向可能存在的冲击前沿和东南方向的冷前沿特征。结合星系光密度图,我们提出了一个弱合并方案。一个年轻的子星系团从东南向西北方向穿过,可以解释光学子峰、ICM温度图、X射线表面亮度过剩和X射线峰偏移。
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Weak Merging scenario of the CLASH Cluster A209
We study the structural and dynamical properties of Abell 209 based on Chandra and XMM-Newton observations. We obtain detailed temperature, pressure and entropy maps with the contour binning method, and find a hot region in the NW direction. The X-ray brightness residual map and corresponding temperature profiles reveal a possible shock front in the NW direction and a cold front feature in the SE direction. Combing with the galaxy luminosity density map we propose a weak merger scenario. A young sub-cluster passing from the SE to NW direction could explain the optical subpeak, the ICM temperature map, the X-ray surface brightness excess, and the X-ray peak offset togethe.
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