Free Access

Fig. 6


Properties of different spectral types of AGN as a function of density contrast. We can see that the stellar mass drops with the density due to gas stripping and high density objects show a stronger starburst and younger stellar populations. The line in C = 2.6 separates the early- and late-type galaxies, showing that Seyferts and LINERs are found in early-type hosts. The left panels show that AGN properties are more dependent on the density than on the web-type.

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.