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The mass profile of early-type galaxies in overdense environments: the case of the double source-plane gravitational lens SL2SJ02176-0513

机译:密集环境中早期星系的质量分布:双源平面引力透镜SL2SJ02176-0513

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Context. The Strong Lensing Legacy Survey (SL2S) provides a sample of the strong lensing events associated with massive distant galaxies, some of which lie in the outskirts of galaxy groups and clusters. Aims. We investigate the internal structure of early-type galaxies in overdense environments, where tidal forces are expected to alter dark matter haloes of infalling galaxies. Methods. SL2SJ02176-0513is a remarkable lens for the presence of two multiply-imaged systems at different redshifts lensed by a foreground massive galaxy at :a bright cusp arc at and an additional double-image system at an estimated redshift of based on photometry and lensing geometry. The system is located about 400kpc away from the centre of a massive group of galaxies. Mass estimates for the group are available from X-ray observations and satellite kinematics. Multicolour photometry provides an estimate of the stellar mass of the main lens galaxy. The lensing galaxy is modelled with two components (stars and dark matter), and we include the perturbing effect of the group environment and all available constraints. Results. We find that classic lensing degeneracies, e.g. between external convergence and mass density slope, are significantly reduced with respect to standard systems and infer tight constraints on the mass density profile: (i) the dark matter content of the main lens galaxy is in line with that of typical galaxies ;(ii) the required mass associated with the dark matter halo of the nearby group is consistent with X-ray (); (iii) accounting for the group contribution in the form of an external convergence, the slope of the mass density profile of the main lens galaxy alone is found to be ,consistent with the isothermal ()slope. Conclusion. We demonstrate that multiple source plane systems together with good ancillary dataset can be used to disentangle local and environmental effects. Key words: gravitational lensing - Galaxy: general - dark matter
机译:上下文。强视力遗产调查(SL2S)提供了与大量遥远星系相关的强视力事件的示例,其中一些星系位于星系群和星团的郊区。目的我们调查了密度过大的环境中早期类型星系的内部结构,在这些环境中,潮汐力有望改变落入星系的暗物质晕圈。方法。 SL2SJ02176-0513是一款出色的镜头,适用于两个不同的红移系统,分别由前景巨大的星系在以下位置产生两个倍增成像系统:明亮的尖端弧形和一个附加的双像系统,其基于光度法和透镜几何估计的红移。该系统距离庞大的星系中心约400kpc。该小组的质量估计数可从X射线观测和卫星运动学获得。多色光度法可以估算主透镜星系的恒星质量。镜头星系是用两个分量(恒星和暗物质)建模的,我们包括了群环境的摄动效应和所有可用的约束。结果。我们发现经典的镜头简并性例如相对于标准系统而言,外部会聚度与质量密度斜率之间的差异显着降低,并推断出对质量密度分布的严格限制:(i)主透镜星系的暗物质含量与典型星系的含量一致;(ii)与附近一组暗物质晕相关的所需质量与X射线()一致; (iii)考虑到外部会聚形式的基团贡献,发现仅主透镜星系的质量密度曲线的斜率与等温()斜率一致。结论。我们证明了多个源平面系统以及良好的辅助数据集可用于解开局部和环境影响。关键词:引力透镜-银河系:一般-暗物质

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