We present a statistical study of X-ray cavities in 77 CC and 112 NCC Planck selected clusters using Chandra observations to further insight into how AGN feedback operates on clusters. The Planck cluster sample is an all-sky mass-selected, nearly unbiased sample of galaxy clusters at moderate redshift (z<0.5), which could reflect the entire AGN feedback cycle at the centers of galaxy clusters. We find that the AGN heating traced by the power of the X-ray cavities alone is able to balance the radiative losses of the ICM in our sample. Our observations show a hint on how the dynamical state of the clusters could affect the asymmetries of the cavities. We also found that clusters with cavities also display Halpha emission, indicating the impor...
Galaxy clusters contain supermassive black holes at their centers. When these supermassive black hol...
The Chandra X-ray Observatory has revealed X-ray bubbles in the intracluster medium (ICM) of many ne...
High-z protoclusters are ideal laboratories to investigate the relation between AGN feedback, ICM he...
International audienceWe study active galactic nucleus (AGN) feedback in nearby (z<0.35) galaxy clus...
We present Chandra X-ray Observatory observations of the core of the galaxy cluster PKS 0745–191. It...
We study active galactic nucleus (AGN) feedback in nearby (z < 0.35) galaxy clusters from the Planck...
We present the first statistical study of X-ray cavities in distant clusters of galaxies (z> 0.3)...
Observations of X-ray jets and cavities in clusters of galaxies observed by Chandra are briefly revi...
X-ray cavities are key tracers of mechanical (or radio mode) heating arising from the active galacti...
20X-ray cavities are key tracers of mechanical (or radio mode) heating arising from the active galac...
In the last two decades, significant improvements have been made in the understanding of how AGN fee...
In the last two decades, significant improvements have been made in the understanding of how AGN fee...
The Chandra X-ray Observatory has revealed X-ray cavities in many nearby cooling flow clusters. The ...
The current generation of flagship X-ray missions, Chandra and XMM-Newton, has changed our understan...
Clusters of galaxies probe the large-scale distribution of matter and are a useful tool to test the ...
Galaxy clusters contain supermassive black holes at their centers. When these supermassive black hol...
The Chandra X-ray Observatory has revealed X-ray bubbles in the intracluster medium (ICM) of many ne...
High-z protoclusters are ideal laboratories to investigate the relation between AGN feedback, ICM he...
International audienceWe study active galactic nucleus (AGN) feedback in nearby (z<0.35) galaxy clus...
We present Chandra X-ray Observatory observations of the core of the galaxy cluster PKS 0745–191. It...
We study active galactic nucleus (AGN) feedback in nearby (z < 0.35) galaxy clusters from the Planck...
We present the first statistical study of X-ray cavities in distant clusters of galaxies (z> 0.3)...
Observations of X-ray jets and cavities in clusters of galaxies observed by Chandra are briefly revi...
X-ray cavities are key tracers of mechanical (or radio mode) heating arising from the active galacti...
20X-ray cavities are key tracers of mechanical (or radio mode) heating arising from the active galac...
In the last two decades, significant improvements have been made in the understanding of how AGN fee...
In the last two decades, significant improvements have been made in the understanding of how AGN fee...
The Chandra X-ray Observatory has revealed X-ray cavities in many nearby cooling flow clusters. The ...
The current generation of flagship X-ray missions, Chandra and XMM-Newton, has changed our understan...
Clusters of galaxies probe the large-scale distribution of matter and are a useful tool to test the ...
Galaxy clusters contain supermassive black holes at their centers. When these supermassive black hol...
The Chandra X-ray Observatory has revealed X-ray bubbles in the intracluster medium (ICM) of many ne...
High-z protoclusters are ideal laboratories to investigate the relation between AGN feedback, ICM he...