We present X-ray and multi-frequency radio observations of the central radio sources in several X-ray cavity systems. We show that targeted radio observations are key to determining if the lobes are being actively fed by the central AGN. Low frequency observations provide a unique way to study both the lifecycle of the central radio source as well as its energy input into the ICM over several outburst episodes
20X-ray cavities are key tracers of mechanical (or radio mode) heating arising from the active galac...
Context. Thermal gas in the center of galaxy clusters can show substantial motions that generate sur...
Measurements of the quantity of radio-mode feedback injected by an active galactic nucleus into the ...
A Chandra image of the central 100 kpc of the Abell 2597 cluster of galaxies shows bright, irregular...
We present new, high resolution radio images of sources associated with cD galaxies and X-ray cavity...
We present LOFAR observations at 120-168 MHz of 42 systems with possible X-ray cavities in their hot...
Gayoung Chon, Hans Böhringer, Martin Krause, and Joachim Trümper, 'Discovery of an X-ray cavity near...
Low frequency radio astronomy allows us to observe the fainter and older synchrotron emission from t...
In this paper we analyze AGN activity signatures in the rich nearby galaxy cluster Abell 1795 aiming...
We present the first Chandra detection of a single X-ray cavity within the interstellar medium of t...
Chandra images of galaxy clusters have revealed a wealth of structure unseen by previous generations...
Outbursts from active galactic nuclei (AGN) can inflate cavities in the intracluster medium (ICM) of...
A 227 ksec Chandra Observatory X-ray image of the hot plasma in the Hydra A cluster has revealed an ...
Original paper can be found at: http://www.astrosociety.org/pubs/cs/381.html Copyright ASPWe present...
none15We present new Giant Metrewave Radio Telescope observations at 235 MHz and 610 MHz of 18 X-ray...
20X-ray cavities are key tracers of mechanical (or radio mode) heating arising from the active galac...
Context. Thermal gas in the center of galaxy clusters can show substantial motions that generate sur...
Measurements of the quantity of radio-mode feedback injected by an active galactic nucleus into the ...
A Chandra image of the central 100 kpc of the Abell 2597 cluster of galaxies shows bright, irregular...
We present new, high resolution radio images of sources associated with cD galaxies and X-ray cavity...
We present LOFAR observations at 120-168 MHz of 42 systems with possible X-ray cavities in their hot...
Gayoung Chon, Hans Böhringer, Martin Krause, and Joachim Trümper, 'Discovery of an X-ray cavity near...
Low frequency radio astronomy allows us to observe the fainter and older synchrotron emission from t...
In this paper we analyze AGN activity signatures in the rich nearby galaxy cluster Abell 1795 aiming...
We present the first Chandra detection of a single X-ray cavity within the interstellar medium of t...
Chandra images of galaxy clusters have revealed a wealth of structure unseen by previous generations...
Outbursts from active galactic nuclei (AGN) can inflate cavities in the intracluster medium (ICM) of...
A 227 ksec Chandra Observatory X-ray image of the hot plasma in the Hydra A cluster has revealed an ...
Original paper can be found at: http://www.astrosociety.org/pubs/cs/381.html Copyright ASPWe present...
none15We present new Giant Metrewave Radio Telescope observations at 235 MHz and 610 MHz of 18 X-ray...
20X-ray cavities are key tracers of mechanical (or radio mode) heating arising from the active galac...
Context. Thermal gas in the center of galaxy clusters can show substantial motions that generate sur...
Measurements of the quantity of radio-mode feedback injected by an active galactic nucleus into the ...