Cosmic Web: Origin and Observables

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dc.creatorPogosyan, D.
dc.creatorBond, J. R.
dc.creatorKofman, L.
dc.creatorWadsley, J.
dc.date1998-10-05
dc.date.accessioned2026-07-07T02:28:14Z
dc.date.available2026-07-07T02:28:14Z
dc.descriptionSimple analytic arguments are used to understand the predominantly filamentary web in the large-scale distribution of galaxies. Numerical simulations of superclusters are performed to assess the feasibility of directly mapping the intracluster webbing, in particular with weak gravitational lensing using Wide Field Cameras.
dc.description6 pages, LaTeX, 5 figures, uses conf_iap.sty To appear in Proceedings of the XIV IAP Colloquium "Wide Field Surveys in Cosmology", eds. S. Colombi and Y. Mellier, Paris, May 26-30 1998. Text and colour figures also available at ftp://ftp.cita.utoronto.ca/pogosyan/cita-98-39
dc.identifierhttps://arxiv.org/abs/astro-ph/9810072
dc.identifierhttp://arxiv.org/abs/astro-ph/9810072
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/13033
dc.subjectAstrophysics
dc.titleCosmic Web: Origin and Observables
dc.typetext

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