Free Access

Fig. 10


Comparison of flaring in the Sco-like and Cyg-like sources using 15 years of RXTE All SKy Monitor data. The peaks in the Cyg X-2 lightcurve are due to source variability, not flaring (see text).

This figure is made of several images, please see below:

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.