Modeling Observational Signatures of Disk-Driven Outflows

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dc.creatorEverett, J. E.
dc.creatorKonigl, A.
dc.creatorKartje, J. F.
dc.date2000-10-12
dc.date.accessioned2026-07-07T01:55:57Z
dc.date.available2026-07-07T01:55:57Z
dc.descriptionWe present a self-consistent, semi-analytical dynamical model of disk driven outflows in AGNs that are accelerated by a combination of magnetic stresses and radiation pressure. This model will make it possible to examine scenarios in which the wind is homogeneous as well as cases where it consists of dense clouds embedded in a more tenuous, magnetized medium. The various ingredients of this model will be tested through quantitative predictions from both multiwavelength spectral observations and reverberation mapping of AGNs.
dc.description7 pages, 2 figures, to appear in "Probing the Physics of AGN by Multiwavelength Monitoring", eds. B.M. Peterson, R.S. Polidan, and R.W. Pogge, ASP Conference Series
dc.identifierhttps://arxiv.org/abs/astro-ph/0010246
dc.identifierhttp://arxiv.org/abs/astro-ph/0010246
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/1831
dc.subjectAstrophysics
dc.titleModeling Observational Signatures of Disk-Driven Outflows
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