Fig. 3.

Distribution of host galaxy axial ratios of INTEGRAL AGN differentiated into broad lines or type 1 i.e. Sy 1−1.2−1.5 (upper and lower left panels), and narrow lines or type 2 i.e. Sy 1.8−1.9−2 (upper and lower right panels). Lower panels: the morphological type of our sample sources has been considered; histograms in dotted red lines refer to AGN hosted in late type (spirals) galaxies, blue dashed lines refer to AGN hosted in early (elliptical and S0) galaxies, and black solid lines refer to host galaxies for which no morphological type has been found in the literature.
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.