Multidimensional analysis of the large-scale segregation of luminosity

Details Multidimensional analysis of the large-scale segregation of luminosity Multidimensional analysis of the large-scale segregation of luminosity

Apr 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apj...339l...9d&link_type=abstract

Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 339, April 1, 1989, p. L9-L11. Research supported by the Direccio

Astronomy and Astrophysics

Astrophysics

23

Cosmology, Galactic Clusters, Luminosity, Astronomical Catalogs, Fractals, Red Shift

Scientific paper

The multidimensional or multifractal formalism has been applied to analyze the CfA catalog. The spectrum of scaling indices and the generalized dimensions D(q) have been found to be scale-invariant in certain scaling regions. This invariance means that the multidimensional formalism is a good tool to characterize galaxy distributions. By means of this formalism it has been found that CfA galaxies brighter than about M(c) = -20(H0 = 100 km/s/Mpc) are most clustered than fainter galaxies.

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