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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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