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in “Clustering in the Universe: from Highly Nonlinear Structures to Homogeneity

By L Guzzo and Osservatorio Astronomico Di Brera


This chapter 1 concentrates on a few specific topics concerning the distribution of galaxies on scales from 0.1 to nearly 1000 h −1 Mpc. The main aim is to provide the reader with the information and tools to familiarize with a few basic questions: 1) What are the scaling laws followed by th

Year: 2001
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