English

Galaxy number counts and Fractal correlations

Astrophysics 2009-10-30 v1

Abstract

We report the correlation analysis of various redshift surveys which shows that the available data are consistent with each other and manifest fractal correlations (with dimension D2D \simeq 2) up to the present observational limits (150\hmp\approx 150 \hmp) without any tendency towards homogenization. This result points to a new interpretation of the number counts that represents the main subject of this letter. We show that an analysis of the small scale fluctuations allows us to reconcile the correlation analysis and the number counts in a new perspective which has a number of important implications.

Keywords

Cite

@article{arxiv.astro-ph/9706106,
  title  = {Galaxy number counts and Fractal correlations},
  author = {M. Montuori and F. Sylos Labini and A. Gabrielli and A. Amici and L. Pietronero},
  journal= {arXiv preprint arXiv:astro-ph/9706106},
  year   = {2009}
}

Comments

Latex file 7 pages and 3 Postscipt figures. Accepted for publication in Europhysics Letters. This paper is also available at http://www.phys.uniroma1.it/DOCS/PIL/pil.html

R2 v1 2026-07-22T09:34:01.171Z