Dynamical Voronoi tessellation. III - The distribution of galaxies

Details Dynamical Voronoi tessellation. III - The distribution of galaxies Dynamical Voronoi tessellation. III - The distribution of galaxies

Jun 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991a%26a...246..291z&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 246, no. 2, June 1991, p. 291-300.

Astronomy and Astrophysics

Astrophysics

8

Astronomical Models, Fractals, Galactic Clusters, Galactic Structure, Galactic Evolution, Red Shift, Three Dimensional Models

Scientific paper

In order to explain the observed three-dimensional structure of galaxies an approximate method is applied to derive the cells belonging to the tessellation. When a fractal distribution of seeds is considered the resulting network of vertices turns out to be fractal with a dimension similar to that of the seeds. More complex distributions are considered in order to simulate the CFA data and the regular spacing of the megawalls.

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