Anisotropic AGN Outflows Filling The Cosmological Volume

dc.creatorBarai, Paramita
dc.creatorGermain, Joel
dc.creatorMartel, Hugo
dc.date2008-09-02
dc.date.accessioned2026-07-07T10:00:13Z
dc.date.available2026-07-07T10:00:13Z
dc.descriptionWe simulate anisotropic outflows of AGN, and investigate the large-scale impact of the cosmological population of AGN outflows over the Hubble time by performing N-body LambdaCDM simulations. Using the observed quasar luminosity function to get the redshift and luminosity distribution, and analytical models for the outflow expansion, AGNs are allowed to evolve in a cosmological volume. By the present epoch, 13 - 25% of the total volume is found to be pervaded by AGN outflows, with 10^{-9} G magnetic field.
dc.description4 pages, 2 figures. Contributed talk at conference "The Central Kiloparsec: Active Galactic Nuclei and Their Hosts", Ierapetra, Crete, 4-6 June 2008. To appear in Volume 79 of the Memorie della Societa Astronomica Italiana
dc.identifierhttps://arxiv.org/abs/0809.0515
dc.identifierhttp://arxiv.org/abs/0809.0515
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/168271
dc.subjectAstrophysics
dc.titleAnisotropic AGN Outflows Filling The Cosmological Volume
dc.typetext

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