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Linking star formation and environment in supercluster galaxies

机译:将星形形成和环境连接在超级群星际星系中

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We present a unique multiwavelength dataset of the Abell 901/902 supercluster at z = 0,16, The environment of the structure is well characterized by weak lensing analysis, galaxy dynamics, and X-ray imaging, and we examine how galaxy properties correlate with these measures of environment We examine the star-formation-density relation and find a surface mass density threshold above which star-formation in supercluster galaxies is truncated, and that this transformation affects primarily the faint end of the star-forming galaxy population (down to M* +6). In addition, we present a preliminary dynamical analysis of the spectroscopic sample (n ~ 300 galaxies), revealing a bimodal distribution of galaxy velocities and significant substructure.
机译:我们在Z = 0,16上呈现ABELL 901/902超级集团的独特多波长数据集,该环境的环境很好地具有弱镜头分析,银河动力学和X射线成像,以及我们如何如何如何关联星系与这些环境措施我们研究了星形成密度关系,并找到了超级簇星系中的星形成的表面质量密度阈值,并且该转化主要影响星形星系群的微弱末端(向下m * +6)。此外,我们提出了对光谱样品(N〜300个星系)的初步动态分析,揭示了星系速度和显着的子结构的双峰分布。

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