Fig. 7
Comparison of the post-outburst high-resolution X-ray spectra of V382 Vel (think black histogram), RS Oph (that was an SSa during outburst, thick red histogram), and the low-inclination system T Pyx (grey shadings). The emission lines in V382 Vel and RS Oph originate in the radiatively cooling ejecta after the novae had turned off. (The concept is the same as described in Fig. 2.)
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.