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A&A 367, 449-456 (2001)
DOI: 10.1051/0004-6361:20000449
Relativistic corrections to fractal analyses of the galaxy distribution
M.-N. Célérier1 and R. Thieberger21 Département d'Astrophysique Relativiste et de Cosmologie, Observatoire de Paris-Meudon, 5 place Jules Janssen, 92195 Meudon Cedex, France
2 Physics Department, Ben Gurion University, Beer Sheva 84105, Israel
e-mail: thieb@bgumail.bgu.ac.il
(Received 3 July 2000 / Accepted 14 November 2000 )
Abstract
The effect of curvature on the results of fractal analyses of the galaxy
distribution is investigated. We show that, if the universe satisfies the
criteria of a wide class of parabolic homogeneous models, the observers
measuring the fractal index with the integrated conditional density
procedure may use the Hubble formula, without having to allow for
curvature, out to distances of 600 Mpc, and possibly far beyond. This
contradicts a previous claim by Ribeiro (1995) that, in the
Einstein-de Sitter case, relativistic corrections should be taken into
account at much smaller scales. We state for the class of cosmological
models under study, and give grounds for conjecture for others,
that the averaging procedure has a smoothing effect and that,
therefore, the redshift-distance relation provides an upper limit to the
relativistic corrections involved in such analyses.
Key words: galaxies: general -- relativity
Offprint request: M.-N. Célérier, Marie-Noelle.Celerier@obspm.fr
© ESO 2001
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