Measuring cavity powers of active galactic nuclei in clusters using a hybrid X-ray–radio method - A new window on feedback opened by subarcsecond LOFAR-VLBI observations

Open Access

Fig. 5.

Hybrid X-ray–radio cavity power measurements versus the purely X-ray-based cavity power estimates. The blue data points indicate the measurements derived using high-resolution observations, while the black data points indicate the measurements derived using low-resolution observations.

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