Density profiles and clustering of dark halos and clusters of galaxies

dc.creatorSuto, Yasushi
dc.date2002-07-09
dc.date.accessioned2026-07-07T02:04:14Z
dc.date.available2026-07-07T02:04:14Z
dc.descriptionDensity profiles of cosmological virialized systems, or dark halos, have recently attracted much attention. I first present a brief historical review of numerical simulations to quantify the halo density profiles. Then I describe the latest results on the universal density profile and their observational confrontation. Finally I discuss a clustering model of those halos with particular emphasis on the cosmological light-cone effect.
dc.descriptioninvited review to appear in the proceedings of "Matter and Energy in Clusters of Galaxies", edited by S. Bowyer and C.-Y. Hwang
dc.identifierhttps://arxiv.org/abs/astro-ph/0207202
dc.identifierhttp://arxiv.org/abs/astro-ph/0207202
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/4674
dc.subjectAstrophysics
dc.titleDensity profiles and clustering of dark halos and clusters of galaxies
dc.typetext

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