Higher-order superclustering in the Ostriker explosion scenario. I - Three-point correlation functions of clusters in the constant and power-law models

Details Higher-order superclustering in the Ostriker explosion scenario. I - Three-point correlation functions of clusters in the constant and power-law models Higher-order superclustering in the Ostriker explosion scenario. I - Three-point correlation functions of clusters in the constant and power-law models

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990a%26a...233....7j&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 233, no. 1, July 1990, p. 7-15.

Statistics

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1

Computational Astrophysics, Dark Matter, Galactic Clusters, Power Series, Astronomical Models, Correlation, Cosmology, Galactic Structure, String Theory

Scientific paper

Three-point correlation functions of clusters in two types of explosion models are discussed. The shells are assumed to have a constant radii or have power law radius distributions. More detailed studies of r-, u-, and v-dependences of Q show that Q remains constant in the constant models. In the power models, Q is independent of the shape parameters u and v, while it has some moderate r-dependences.

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