Free Access
Table 1
Parametrization of the AGN model.
| Component | Description |
|
|
|
| Continuum sources | 2 point-like sources of isotropic emission, |
| power-law spectrum with a spectral flux F∗ ∝ ν− α, | |
| photon index Γ = 1+α = variable, | |
| distance from accretion disk mid-plane = ± 1 × 10-3 pc | |
|
|
|
| Accretion disk | cylindrical disk with Rout = 4 × 10-3 pc, |
| half-thickness = 3.25 × 10-7 pc, | |
| irradiated by two isotropic sources, | |
| filled with optically thick cold matter | |
|
|
|
| Equatorial hot flow | wedge structure with Rin = 3 × 10-2 pc and Rout = 5 × 10-2 pc, |
| half-opening angle (from the equatorial plane) = 20°, | |
| equatorial Thomson optical depth = 1, | |
| filled with electrons | |
|
|
|
| Polar outflows | double-cone with Rin = 1 pc and Rout = 400 pc, |
| half-opening angle (from the polar axis) = 33°, | |
| vertical Thomson optical depth = 0.3, | |
| filled with electrons | |
|
|
|
| Dusty torus | elliptical torus with Rin = variable and Rout = 2.0 pc, |
| half-opening angle (from the polar axis) = variable, | |
| equatorial Mie optical depth ≫ 1, | |
| filled with optically-thick cold matter | |
Notes. Parametrization of the AGN model used in this paper (references are given in the text). A sketch of the model can be seen in Fig. 1.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.