Observations of X-ray jets and cavities in clusters of galaxies observed by Chandra are briefly reviewed. A recent study on the excess of central gas entropy, which can be considered as direct evidence for AGN feedback in galaxy groups and clusters is presented. An expanded account of this study has been presented in RAA (Wang et al. 2010)
As a part of an ongoing study of a sample of galaxy groups showing evidence for AGN/hot gas interact...
Observations with the ChandraX-ray Observatory are used to examine the hot gas properties within a s...
X-ray cavities are key tracers of mechanical (or radio mode) heating arising from the active galacti...
We present a statistical study of X-ray cavities in 77 CC and 112 NCC Planck selected clusters using...
We present gas temperature, density, entropy and cooling time profiles for the cores of a sample of ...
Observations with the ChandraX-ray Observatory are used to examine the hot gas properties within a s...
Observations with the ChandraX-ray Observatory are used to examine the hot gas properties within a s...
The current generation of flagship X-ray missions, Chandra and XMM-Newton, has changed our understan...
Observations with the ChandraX-ray Observatory are used to examine the hot gas properties within a s...
Observations with the ChandraX-ray Observatory are used to examine the hot gas properties within a s...
Observations with the ChandraX-ray Observatory are used to examine the hot gas properties within a s...
Observations with the ChandraX-ray Observatory are used to examine the hot gas properties within a s...
As a part of an ongoing study of a sample of galaxy groups showing evidence for AGN/hot gas interact...
Context. In the last few years, the outskirts of galaxy clusters have been studied in detail and the...
Context. In the last few years, the outskirts of galaxy clusters have been studied in detail and the...
As a part of an ongoing study of a sample of galaxy groups showing evidence for AGN/hot gas interact...
Observations with the ChandraX-ray Observatory are used to examine the hot gas properties within a s...
X-ray cavities are key tracers of mechanical (or radio mode) heating arising from the active galacti...
We present a statistical study of X-ray cavities in 77 CC and 112 NCC Planck selected clusters using...
We present gas temperature, density, entropy and cooling time profiles for the cores of a sample of ...
Observations with the ChandraX-ray Observatory are used to examine the hot gas properties within a s...
Observations with the ChandraX-ray Observatory are used to examine the hot gas properties within a s...
The current generation of flagship X-ray missions, Chandra and XMM-Newton, has changed our understan...
Observations with the ChandraX-ray Observatory are used to examine the hot gas properties within a s...
Observations with the ChandraX-ray Observatory are used to examine the hot gas properties within a s...
Observations with the ChandraX-ray Observatory are used to examine the hot gas properties within a s...
Observations with the ChandraX-ray Observatory are used to examine the hot gas properties within a s...
As a part of an ongoing study of a sample of galaxy groups showing evidence for AGN/hot gas interact...
Context. In the last few years, the outskirts of galaxy clusters have been studied in detail and the...
Context. In the last few years, the outskirts of galaxy clusters have been studied in detail and the...
As a part of an ongoing study of a sample of galaxy groups showing evidence for AGN/hot gas interact...
Observations with the ChandraX-ray Observatory are used to examine the hot gas properties within a s...
X-ray cavities are key tracers of mechanical (or radio mode) heating arising from the active galacti...