Simulations of the Local Universe

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dc.creatorGottloeber, Stefan
dc.creatorKlypin, Anatoly
dc.creatorKravtsov, Andrey
dc.creatorHoffman, Yehuda
dc.creatorFaltenbacher, Andreas
dc.date2002-08-21
dc.date.accessioned2026-07-07T02:04:46Z
dc.date.available2026-07-07T02:04:46Z
dc.descriptionThe theory of structure formation predicts that galaxies form within extended massive dark matter halos built from smaller pieces that collided and merged, resulting in the hierarchy of galaxies, groups, and clusters observed today. Here we present constrained numerical simulations designed to match the observed local universe as well as possible and to study the formation, evolution and present day properties of such dark matter halos in different environments. Simulations have been done with different versions of the Adaptive Refinement Tree (ART) N-body code, some of them including eulerian gasdynamics.
dc.description10 pages, 6 figures, to appear in the proceedings of the "First Joint HLRB and KONWIHR Result and Reviewing Workshop" (Munich, October 2002). Version with high resolution figures available at http://www.aip.de/People/SGottloeber/papers/h009za.ps.gz (gzipped 5.3 Mb)
dc.identifierhttps://arxiv.org/abs/astro-ph/0208398
dc.identifierhttp://arxiv.org/abs/astro-ph/0208398
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/4887
dc.subjectAstrophysics
dc.titleSimulations of the Local Universe
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