The angular projection of fractals and its relevance for the galaxy distributions

Details The angular projection of fractals and its relevance for the galaxy distributions The angular projection of fractals and its relevance for the galaxy distributions

Feb 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991phya..171..239d&link_type=abstract

Physica A, Volume 171, Issue 2, p. 239-248.

Physics

5

Scientific paper

The distribution of points corresponding to the angular projection of a fractal is shown to become homogeneous for relatively large angels. In addition the corresponding correlation function w(θ) depends strongly on the angular half-width of the considered sample. These results show that, contrary to the usual interpretation, the observed angular correlations of galaxies can actually be compatible with a fractal structure in space.

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