Delving into the depths of NGC 3783 with XRISM - I. Kinematic and ionization structure of the highly ionized outflows

Open Access

Fig. 3.

Transmission model of the six outflow components. The spectra correspond to the best-fit model parameters of Table 1. Components are labeled with a letter in increasing order of the outflow velocity (v_out), and those with similar v_out are further sub-labeled by a number in decreasing order of the ionization parameter (ξ).

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.