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Constraints on the broad-line region properties and extinction in local Seyferts

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Academic year: 2021

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Table 1. Summary of the observations, Seyfert sub-types (see Section 3.4), 14–195 keV luminosity (taken from Davies et al
Table 3. Best-fitting parameters H and n H . Abbreviated name:
Figure 2. Ionizing photon flux H versus hydrogen number density n H . The diamonds indicate the location of our AGN in the plane, as shown in Fig
Table 5. Distance from the nucleus to the broad H I emitting region in terms of the dust sublimation radius (see Section 4.1 for details).
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