Fig. 7
Variation in the main oscillation frequency (mode a) of the X-ray light curve as a function of the white dwarf mass, for different accretion rates in the case of pure bremsstrahlung cooling. The curves represent the best fits following the theoretical tendency given by the relation (19).
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.