Searching for similarities in the accretion flow of Seyfert 1 galaxies and cataclysmic variables based on the flare profiles of IRAS 13224–3809, 1H 0707–495, Mrk 766, and MV Lyr

Open Access

Fig. 7.

Comparison of IRAS 13224–3809 AFPs in the soft and hard bands together with that from the whole energetic interval. The left panel represents the same as Fig. 4, and the right panel only compares high-flux intervals, like in Fig. 6.

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.