Fig. 7
XMM-Newton/RGS spectra obtained from high (dashed line) and low (solid) flux good time intervals in the 15–17 Å (Fig. 6) region in which several density-sensitive Fe XVII lines are present for OBS2 and OBS3. The generally greater strengths of these lines and the 16.8 Å/17.0 Å ratio are discussed in the text. These spectra are smoothed over two 2 mÅ bins.
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.