Dynamical Voronoi tessellation. II - The three-dimensional case

Details Dynamical Voronoi tessellation. II - The three-dimensional case Dynamical Voronoi tessellation. II - The three-dimensional case

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990a%26a...233..293z&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 233, no. 1, July 1990, p. 293-300.

Statistics

Computation

3

Galactic Clusters, Interstellar Matter, Plasma Bubbles, Supernova Remnants, Computational Astrophysics, Galactic Nuclei, Normal Density Functions

Scientific paper

For a given configuration of nuclei in a three-dimensional space, a procedure for constructing the corresponding Voronoi diagram is presented. A similar procedure is derived to explore the case in which the signals starting from the nuclei are still expanding. The theory is tentatively applied to the SN explosions in the Galactic center and to the cluster's arcs.

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