Transient phenomena and cluster formation

Details Transient phenomena and cluster formation Transient phenomena and cluster formation

Nov 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990a%26a...239....1z&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 239, no. 1-2, Nov. 1990, p. 1-6.

Statistics

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4

Correlation Coefficients, Galactic Clusters, Galactic Evolution, Mass Distribution, Astronomical Models, Computational Astrophysics, Random Processes, Transient Response

Scientific paper

The tendency to form clusters in a random process through explosions is investigated. Using a hierarchical model in which structures at different scales are generated by explosions of 'seeds', with each seed being a structure in the previous (larger) scale, the form of the correlation coefficient of the clusters, superclusters, and galaxies is determined. It is shown that structures generated by different-scale explosions could produce a fractal distribution on hierarchical scales similar to those observed.

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