Free Access

Fig. 5


Broad-band optical/NIR to X-ray SEDs fitted with a broken power-law with the sharp break (top left) and with a broken power-law with the smooth break (bottom left). Best-fit power-law fits to the temporal evolution of the cooling-break energy are shown on the right, resulting from the sharp (top) and the smooth (bottom) broken power-law fits.

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.