The XMM-Newton and NuSTAR view of IRASF11119+3257 - I. Detection of multiple ultra fast outflow components and a very cold corona

Open Access

Fig. 7.

XMM-Newton and NuSTAR spectra with the best-fit continuum model and residuals, for the model described in Sect. 6.2, where the DISK-WIND table replaces the UFO_H XSTAR table. The colors are the same as in Figure 1.

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.