R. P. Deo

TL;DR: In this article, the authors explore self-similar, dusty disk winds, driven by both magnetocentrifugal forces and radiation pressure, as an explanation for the torus and make predictions of AGN infrared (IR) spectral energy distributions from 2 to 100 µm by varying parameters such as the viewing angle (from i = 0 Degree-Sign to 90 degree-Sign ), the base column density of the wind, the Eddington ratio (from L/L{sub Edd} = 0.01 to 0.1), the black hole mass (from M{sub

TL;DR: In this paper, the authors explore self-similar, dusty disk-winds, driven by both magnetocentrifugal forces and radiation pressure, as an explanation for the torus and make predictions of AGN infrared spectral energy distributions (SEDs) from 2-100 microns by varying parameters such as: the viewing angle; the base column density of the wind; the Eddington ratio; the black hole mass; and the amount of power in the input spectrum emitted in the X-ray relative to that emitted in UV/optical.

TL;DR: In this article, the authors explore the connection between these emission-line properties and the UV through X-ray spectral energy distribution (SED) for radio-quiet (RQ) quasars.

TL;DR: In this article, a suite of emission features including high ionization coronal lines from the narrow line region illuminated by the ionizing continuum, broad dust bumps from silicates and graphites, and polycyclic aromatic hydrocarbons (PAH) features from star formation in the host galaxy are detected in most individual spectra.

TL;DR: In this paper, the authors show that large-scale, organized magnetic fields are present in radio-quiet active galactic nuclei and provide evidence for the existence of a dust-wind model for the putative obscuring torus.