Theory of winds in AGNs

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dc.creatorProga, Daniel
dc.date2007-01-04
dc.date.accessioned2026-07-07T07:38:26Z
dc.date.available2026-07-07T07:38:26Z
dc.descriptionI present a brief review of theory of winds in active galactic nuclei (AGN). Magnetic, radiation, and thermal driving likely operate in AGN. In many cases, it is difficult to distinguish, both from observational and theoretical point of view, which of these wind driving mechanisms dominates in producing winds. Therefore, I focus on specific theoretical predictions which could help to improve our understanding of the physics of AGN winds.
dc.description10 pages, conference proceedings to appear in "The Central Engine of Active Galactic Nuclei", ed. L. C. Ho and J.-M. Wang (San Francisco: ASP), invited talk
dc.identifierhttps://arxiv.org/abs/astro-ph/0701100
dc.identifierhttp://arxiv.org/abs/astro-ph/0701100
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/121084
dc.subjectAstrophysics
dc.titleTheory of winds in AGNs
dc.typetext

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