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The Large-Scale Environment of Groups & Clusters of Galaxies

机译:群星群与群星群的大规模环境

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摘要

It appears that the dynamical status of clusters and groups of galaxies isrelated to the large-scale structure of the Universe. A few interesting trendshave been established: (1) The Cluster Substructure - Alignment Connection, by which clusters show astrong correlation between their tendency to be aligned with their neighborsand their dynamical state (as indicated by the existence of significantsubstructres). (2) The Cluster Dynamics -Cluster Clustering Connection, bywhich dynamically young clusters are more clustered than the overall clusterpopulation. (3) The Cluster- Supercluster Alignment Connection, by whichclusters of galaxies show a statistical significant tendency to be aligned withthe projected major axis orientation of their parent supercluster. (4) TheGalaxy Alignment - Cluster Dynamics Connection, by which red-sequence clusterbright galaxies show a significant trend to be aligned with their parentcluster major axis, especially in dynamically young clusters. (5) The GroupRichness - Shape Connection, by which groups of galaxies are flatter the poorerthey are. These are strong indications that clusters develop in a hierarchical fashionby anisotropic merging of smaller units along the large-scale filamentarystructures within which they are embedded.
机译:看来星系团和星团的动力学状态与宇宙的大规模结构有关。已经建立了一些有趣的趋势:(1)群集子结构-对齐连接,通过群集,群集显示出其与邻居对齐的趋势与其动态状态之间的密切相关性(通过显着子结构的存在表明)。 (2)群集动力学-群集群集连接,通过它动态地将年轻的群集比整个群集总体进行群集。 (3)星团-超级团簇对准连接,星系团显示出统计上的显着趋势,即与其父超级团簇的投影主轴方向对准。 (4)“银河系对准-集群动力学连接”,通过该序列,红色序列的集群明亮的星系显示出与其父集群主轴对齐的明显趋势,尤其是在动态年轻的集群中。 (5)GroupRichness-形状连接,星系越平坦,星系越平坦。这些有力的迹象表明,簇是通过沿着嵌入它们的大规模丝状结构将较小的单元各向异性合并而形成的。

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    Plionis, Manolis;

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  • 年度 2004
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