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Table 1.
Components of the NGC 1068 model, its host galaxy and the interstellar polarization.
| Continuum source | |
| Punctual isotropic power-law SED | F * ∝ ν −1 |
| Accretion flow | |
| Inner and outer radii | 0.001–0.1 pc |
| Half-opening angle (from the eq. plane) | 20° |
| Composition and optical depth | electrons (τ V = 1) |
| Circumnuclear region | |
| Inner and outer radii | 0.1–5 pc |
| Half-opening angle (from the eq. plane) | 45° |
| Composition and optical depth | dust (τ V ≥ 50) |
| Biconical polar outflows | |
| Inner and outer radii | 0.1–100 pc |
| Half-opening angle (from the eq. plane) | 45° |
| Composition and optical depth | electrons (τ V = 1) |
| Host galaxy | |
| Template | Sbc |
| Inner and outer radii | 5–3 000 pc (truncated) |
| Interstellar polarization | |
| Polarization degree | 0.5% |
| Polarization angle | 0° |
Notes. See text in Sects. 3.1, 3.2, and 3.3 for details and references.
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