Fig. 1
Absorption measure distribution for the warm absorber of NGC 3783 using the solar chemical abundances measured by Asplund (2009). Top panel: differential form of the AMD. In the bottom panel it is integrated up to the total column density (see Eq. (1)). A scale in ξ and in temperature T are provided with the relation T(ξ) being obtained from the xstar computations of the fractional ionic abundances (see text).
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.