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首页> 外文期刊>Astronomy and astrophysics >Witnessing a merging bullet being stripped in the galaxy cluster RXCJ2359.3-6042
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Witnessing a merging bullet being stripped in the galaxy cluster RXCJ2359.3-6042

机译:目睹星系团RXCJ2359.3-6042中正在剥离的合并子弹

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We report the discovery of the merging cluster, RXCJ2359.3-6042, from the REFLEX II cluster survey and present our results from all three detectors combined in the imaging and spectral analysis of the XMM-Newton data. Also known as Abell 4067, this is a unique system, where a compact bullet penetrates an extended, low density cluster at redshift z = 0.0992 clearly seen from our follow-up XMM-Newton observation. The bullet goes right through the central region of the cluster without being disrupted and we can clearly see how the bullet component is stripped of its layers outside the core. There is an indication of a shock heated region in the east of the cluster with a higher temperature. The bulk temperature of the cluster is about 3.12(±0.13) keV implying a lower mass system. Spearheading the bullet is a cool core centred by a massive early type galaxy. The temperatures and metallicities of a few regions in the cluster derived from the spectral analysis supports our conjecture based on the surface brightness image that a much colder compact component at 1.55(±0.10) keV with large metallicity (0.75 Z⊙) penetrates the main cluster, where the core of the infalling component survived the merger and left stripped gas behind at the centre of the main cluster. We also give an estimate of the total mass within r500, which is about 2 × 1014 M⊙ from the deprojected spherical β modelling of the cluster in good agreement with other mass estimates from the M ? TX and M ? σv relations.
机译:我们报告了从REFLEX II聚类调查中发现的合并聚类RXCJ2359.3-6042,并提出了结合XMM-Newton数据的成像和光谱分析的所有三个探测器的结果。这也称为Abell 4067,这是一个独特的系统,其中紧凑的子弹在红移z = 0.0992时穿透扩展的低密度簇,这从我们的后续XMM-Newton观测清楚可见。子弹正好穿过群集的中央区域而不会受到干扰,我们可以清楚地看到子弹组件如何从核心外部剥离其层。有迹象表明,在星团东部有一个高温加热区。团簇的整体温度约为3.12(±0.13)keV,表明系统质量较低。引领子弹的是一个以庞大的早期星系为中心的酷核心。通过光谱分析得出的团簇中几个区域的温度和金属性基于表面亮度图像支持了我们的推测,即表面温度为1.55(±0.10)keV的冷得多的致密组分穿透了大的金属性(0.75Z⊙) ,下降部分的核心在合并中幸存下来,并在主集群中心留下了剥离的气体。我们还给出了r500内的总质量的估计值,该估计值是通过对簇的投影球面β模型建模得出的约2×1014M⊙,与来自M的其他质量估计值非常吻合。 TX和M? σv关系。

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