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Substructure in dwarf spheroidals — a star cluster connection?

机译:矮小球体的子结构 - 星形集群连接?

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The observational evidence for kinematic substructure in Local Group dSphs isreviewed. The properties of these substructures are consistent with their being disrupted starclusters. The persistence of cold substructure argues strongly against the presence of dark mattercusps in the haloes of dSphs. A formation scenario for dSphs is described involving the mergerof star clusters in the potential well of a low-mass dark matter halo.
机译:本地组DSPS中的运动次结构的观察证据ISREVIEWED。这些子结构的性质与它们被破坏的星形板相一致。冷子结构的持久性强烈地反对DSPS的卤素中的暗物质的存在。描述了DSPH的形成情况,涉及低质量暗物质晕的潜在井中的Mergerof星团。

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