Correlation functions in a filamentary clustering prescription

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Galactic Clusters, Mass Distribution, Spatial Distribution, Statistical Correlation, Astronomical Models, Filaments, Hierarchies, Statistical Distributions

Scientific paper

Two simple clustering prescriptions have provided useful comparisons for studies of the properties of the large-scale galaxy distribution: the power-law cluster model and the continuous hierarchy model. The author proposes another simple paradigm, inherently "filamentary", whose correlation functions scale with size in a way indistinguishable at present from those of the continuous hierarchy. There exists a growing body of observational evidence for filaments.

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