彗星星系团核心的线性结构
J S Sanders1, A C Fabian, E Churazov
1Max-Planck-Institut für Extraterrestrische Physik, Giessenbachstrasse 1, 85748 Garching, Germany. jsanders@mpe.mpg.de
概括
星系团核心表现出大规模结构,挑战流理论. 深度钱德拉X射线观测显示了长寿命,低的手臂,这表明由于磁场的作用抑制了流和导电.
科学领域:
- 天体物理学 天体物理学
- 星系团星系团的星系团
- 等离子体物理学的物理学
背景情况:
- 星系团包含热的X射线发射等离子体.
- 预计这种等离子体中的流运动将对能量密度做出重大贡献.
- 了解等离子体动态对于星团进化至关重要.
研究的目的:
- 调查Coma星团核心中等离子体的结构和动态.
- 确定观察到的等离子体结构的寿命和起源.
- 评估这些结构对流和导电的影响.
主要方法:
- 深月球X射线天文台对Coma星团的观测.
- 分析了跨越150 kiloparsecs的近线性高密度臂.
- 追踪可能从合并子集群中剥离的低材料.
主要成果:
- 在Coma星团核心中发现了广泛,连贯的低臂.
- 确定这些臂和一个合并的星系子组之间的联系.
- 证据表明连贯性超过几亿年.
结论:
- 观测到的结构暗示了集群核心中被抑制的同otropic 流和导电.
- 磁场可能是抑制流和导电的原因.
- 这些发现提供了对过去10亿年的子集群合并活动的见解.
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