Fig. 2.
Lines resulting from the modeling assuming that there is no torus, and assuming both a small Rdiss(=2.25 × 1017 cm) and a large Rdiss(=3.6 × 1018 cm). Parameters are listed in Table 4. If we fit the high-energy emission, the model underproduces the near-IR flux. The long dashed line corresponds to the first- and the second-order Compton SSC contributions.
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.