Observational Support for the Gurzadyan-Kocharyan Relation in Clusters of Galaxies

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dc.creatorMonaco, Pierluigi
dc.date1994-05-31
dc.date.accessioned2026-07-07T02:19:12Z
dc.date.available2026-07-07T02:19:12Z
dc.descriptionWe show that observational data for four Abell clusters of galaxies support the Gur\-za\-dyan-Kocharyan relation between the Hausdorff dimension and the dynamical properties of a galaxy system. The Hausdorff dimension is calculated using the two-point correlation function, while the dynamical parameters are estimated using available data and reasonable assumptions on the mass function of galaxies. This result can have essential consequences in the understanding of the dynamical mechanisms that determine the fractal distribution of galaxies.
dc.description5 pages, uuencoded postscript file with figures, SISSA Preprint 72/94/A, A&A Letters in press
dc.identifierhttps://arxiv.org/abs/astro-ph/9405070
dc.identifierhttp://arxiv.org/abs/astro-ph/9405070
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/9771
dc.subjectAstrophysics
dc.titleObservational Support for the Gurzadyan-Kocharyan Relation in Clusters of Galaxies
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