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We will discuss here how structures observed in clusters of galaxies can provide us insight on the formation and evolution of these objects. We will focus primarily on X-ray observations and results from hydrodynamical -body simulations. This paper is based on a talk given at the School of Cosmology Jose Plinio Baptista – `Cosmological perturbations and Structure Formation’ in Ubu/ES, Brazil.

生成讲解博客的中文版本

生成AI智能校验的中文版本