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fbtwitterlinkedinvimeoflicker grey 14rssslideshare1
F. Sylos Labini; L. Pietronero (1996)
Publisher: Copernicus Publications
Journal: Nonlinear Processes in Geophysics
Languages: English
Types: Article
Subjects: Geophysics. Cosmic physics, Q, [ PHYS.ASTR.CO ] Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], [ SDU.STU ] Sciences of the Universe [physics]/Earth Sciences, Science, Physics, QC1-999, QC801-809, [ SDU.ASTR ] Sciences of the Universe [physics]/Astrophysics [astro-ph]

Classified by OpenAIRE into

arxiv: Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics::Galaxy Astrophysics
The recent availability of complete three dimensional samples of galaxies and clusters permits a direct study of their spatial properties. We present a brief review of galaxy correlations based on the methods modern statistical Physics. These methods which able to identify self-similar and non-analytical prop ties, allow us to test the usual homogeneity assumption of luminous matter distribution. We conclude that both the three dimensional prop ties, and the angular log N - log S relation, point out the fact that the distribution of galaxies and clusters fractal with D ≈ 2 up to the deepest scale probed luminous matter (≈≥ 1000h-1 Mpc). This result has important implications for the theoretical framework that should be adopted.
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