The method of a two-point conditional column density for estimating the fractal dimension of the distribution of galaxies

Astronomy Letters

Volumn 30, Issue 7, 2004, Pages 444-450

  Baryshev, Yu V ^a   Bukhmastova, Yu L ^a  

^a ST PETERSBURG STATE UNIVERSITY   (Russian Federation)

Author keywords

Fractal dimension; Galaxies; Groups and clusters of galaxies; Intergalactic gas; Spatial galaxy distribution

Indexed keywords

EID: 4444317774     PISSN: 10637737     EISSN: None     Source Type: Journal    
DOI: 10.1134/1.1774395     Document Type: Article

References (8)

1. Yu. V. Baryshev and Yu. L. Ezova, Astron. Zh. 74, 497 (1997) [Astron. Rep. 41, 436 (1997)].
2. Yu. V. Baryshev and Yu. L. Ezova, Astron. Zh. 74, 497 (1997) [Astron. Rep. 41, 436 (1997)].
3. A. Gabrielli, F. Sylos Labini, M. Joyce, and L. Pietronero, Statistical Physics for Cosmic Structures (Springer, Berlin, 2004, in press).
4. B. B. Mandelbrot, The Fractal Geometry of Nature (Freeman, New York, 1982).
5. V. J. Martinez and E. Saar, Statistics of the Galaxy Distribution (Chapman & Hall/CRC, New York, 2002).
6. G. Paturel, Astrophys. J., Suppl. Ser 124, 109 (1997).
7. L. Pietronero, Physica A 144, 257 (1987).
8. F. Sylos-Labini, M. Montuori, and L. Pietronero, Phys. Rep. 293, 61 (1998).