Linking Cluster Formation to Large Scale Structure

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dc.creatorColberg, J. M.
dc.creatorWhite, S. D. M.
dc.creatorJenkins, A.
dc.creatorPearce, F. R.
dc.date1997-11-05
dc.date.accessioned2026-07-07T02:24:56Z
dc.date.available2026-07-07T02:24:56Z
dc.descriptionWe use two high resolution CDM simulations to show that (i) when clusters of galaxies form the infall pattern of matter is not random but shows clear features which are correlated in time; (ii) in addition, the infall patterns are correlated with the cluster's surrounding Large Scale Structure; (iii) Large Scale Structure shows a mix of both filaments and sheets; (iv) the amount of mass in filaments is slightly larger for a low $Ω$ model.
dc.description6 pages (incl. 7 figs)
dc.identifierhttps://arxiv.org/abs/astro-ph/9711040
dc.identifierhttp://arxiv.org/abs/astro-ph/9711040
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/11748
dc.subjectAstrophysics
dc.titleLinking Cluster Formation to Large Scale Structure
dc.typetext

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