Free Access

Fig. 4

thumbnail

Left panel: adaptively smoothed Chandra X-ray image (Obs. ID 497) in the 0.2–10 keV band of the galaxy cluster A2199 with the VLA contour levels at 8415 MHz overlaid. Pronounced X-ray cavities can be identified in correspondence of the radio galaxy lobes. Top right panel: deprojected thermal gas density profile (Johnstone et al. 2002). Bottom right panel: pixel distribution of the rotation measure image as a function of the distance from the cluster center.

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.