Free Access
Fig. 4
Theoretical predicted relation between Porb,f and M2,f for binary radio pulsars. The solid curves and dashed curves correspond to the relations obtained by Rappaport et al. (1995) and Tauris & Savonije (1999). The open star sign represents our simulation result.
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.