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Beppo-SAX temperature maps of galaxy clusters in the Corona Borealis supercluster: A2061, A2067 and A2124

机译:北极光晕中星系团的Beppo-saX温度图   超星系团:a2061,a2067和a2124

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摘要

In this paper we present the analysis of Beppo-SAX observations of thecluster pairs A2061-A2067 and A2122-A2124, located in the Corona Borealissupercluster, which have been selected as candidate merging clusters. The aimof this work is to study the physics of the intracluster medium and to look forthe possible presence of merging signatures. We derived the global temperatures and abundances and the temperatureprofiles and maps for these clusters. We do not find any significant evidenceof interaction between the clusters forming the pairs, but we detect acandidate shock inside A2061. On the basis of the X-ray and optical propertiesof this cluster we propose a scenario in which a group is falling inside A2061.This interaction is in the phase in which the cores have not encountered yetand in which the formation of a shock is expected.
机译:在本文中,我们对位于Corona Borealis超级集群中的集群对A2061-A2067和A2122-A2124的Beppo-SAX观测结果进行了分析,这些集群对已被选为候选合并集群。这项工作的目的是研究集群内部介质的物理特性,并寻找可能存在合并签名的情况。我们得出了全球温度和丰度以及这些星团的温度分布图和图。我们没有发现形成该对的簇之间相互作用的任何重要证据,但是我们检测到A2061内部的候选冲击。根据该星团的X射线和光学特性,我们提出了一种情况,其中一个团落在A2061内,这种相互作用处于尚未遇到铁心且预计会形成冲击的阶段。

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