Percolation and synchrotron emission. II - Galaxy distribution

Details Percolation and synchrotron emission. II - Galaxy distribution Percolation and synchrotron emission. II - Galaxy distribution

Apr 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988a%26a...195....1z&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 195, no. 1-2, April 1988, p. 1-8.

Astronomy and Astrophysics

Astrophysics

1

Computerized Simulation, Cosmic Rays, Galactic Clusters, Percolation, Radio Galaxies, Synchrotron Radiation, Energy Dissipation, Galactic Evolution, Random Walk

Scientific paper

The distribution of galaxies, radio galaxies, and their synchrotron emission are investigated theoretically by means of numerical simulations based on the percolation-theory model of Zaninetti (1987). The construction of the model is described, and the results are presented in extensive graphs and briefly characterized. The percolation approach is shown to produce a nonthermal-source distribution with voids and clusters, and to permit graphic display of the appearance (as streaming cosmic rays) of the low-intensity continuum radiation from clusters.

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