Matter Outflows from AGN: A Unifying Model
arXiv:astro-ph/0610003 · doi:10.1007/s10509-006-9180-2
Abstract
We discuss a self-consistent unified model of the matter outflows from AGNs based on a theoretical approach and involving data on AGN evolution and structure. The model includes a unified geometry, two-phase gas dynamics, radiation transfer, and absorption spectrum calculations in the UV and X-ray bands. We briefly discuss several questions about the mass sources of the flows, the covering factors, and the stability of the narrow absorption details.
6 figures, accepted for publication in Astrophysics and Space Science
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