Free Access

Fig. 2


RHD flow in the shocked pulsar wind. The star is at the origin (0,0) and the pulsar is at (1,0) in units of the orbital separation d. A few selected streamlines have been plotted. Three different regions have been coloured. They correspond to the bow shock (blue), the reflected shock (light blue), and the back shock (dark blue) regions.

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.