20We present new, deep observations of the Phoenix cluster from Chandra, the Hubble Space Telescope, and the Karl Jansky Very Large Array. These data provide an order-of-magnitude improvement in depth and/or angular resolution over previous observations at X-ray, optical, and radio wavelengths. We find that the one-dimensional temperature and entropy profiles are consistent with expectations for pure-cooling models. In particular, the entropy profile is well fit by a single power law at all radii, with no evidence for excess entropy in the core. In the inner ∼10 kpc, the cooling time is shorter than any other known cluster by an order of magnitude, while the ratio of the cooling time to freefall time (t cool/t ff) approaches unity, signalin...
The radiative cooling timescales at the centers of hot atmospheres surround-ing elliptical galaxies,...
Context. The relaxed cool-core Phoenix cluster (SPT-CL J2344-4243) features an extremely strong cool...
We present accurate mass and thermodynamic profiles for 57 galaxy clusters observed with the Chandra...
We present new, deep observations of the Phoenix cluster from the Chandra X-ray Observatory, the Hub...
We present first results on the cooling properties derived from Chandra X-ray observations of 83 hig...
Multiwavelength data indicate that the X-ray-emitting plasma in the cores of galaxy clusters is not ...
The classical "cooling flow" model historically associated with "cool core" clusters of galaxies fai...
We present first results on the cooling properties derived from Chandra X-ray observations of 83 hig...
We describe two-dimensional gasdynamical models of jets that carry mass as well as energy to the hot...
© 2018 The Author(s). Active galactic nuclei (AGNs) release a huge amount of energy into the intracl...
Solving the cooling flow problem in cool-core galaxy clusters is critical to under- standing the lar...
Nonradiative simulations that only include heating due to gravitational processes fail to match the ...
It is now widely accepted that heating processes play a fundamental role in galaxy clusters, struggl...
Multiwavelength data indicate that the X-ray emitting plasma in the cores of galaxy clusters is not ...
New Chandra X-ray and Herschel Far-Infrared (FIR) observations enable a multiwavelength study of act...
The radiative cooling timescales at the centers of hot atmospheres surround-ing elliptical galaxies,...
Context. The relaxed cool-core Phoenix cluster (SPT-CL J2344-4243) features an extremely strong cool...
We present accurate mass and thermodynamic profiles for 57 galaxy clusters observed with the Chandra...
We present new, deep observations of the Phoenix cluster from the Chandra X-ray Observatory, the Hub...
We present first results on the cooling properties derived from Chandra X-ray observations of 83 hig...
Multiwavelength data indicate that the X-ray-emitting plasma in the cores of galaxy clusters is not ...
The classical "cooling flow" model historically associated with "cool core" clusters of galaxies fai...
We present first results on the cooling properties derived from Chandra X-ray observations of 83 hig...
We describe two-dimensional gasdynamical models of jets that carry mass as well as energy to the hot...
© 2018 The Author(s). Active galactic nuclei (AGNs) release a huge amount of energy into the intracl...
Solving the cooling flow problem in cool-core galaxy clusters is critical to under- standing the lar...
Nonradiative simulations that only include heating due to gravitational processes fail to match the ...
It is now widely accepted that heating processes play a fundamental role in galaxy clusters, struggl...
Multiwavelength data indicate that the X-ray emitting plasma in the cores of galaxy clusters is not ...
New Chandra X-ray and Herschel Far-Infrared (FIR) observations enable a multiwavelength study of act...
The radiative cooling timescales at the centers of hot atmospheres surround-ing elliptical galaxies,...
Context. The relaxed cool-core Phoenix cluster (SPT-CL J2344-4243) features an extremely strong cool...
We present accurate mass and thermodynamic profiles for 57 galaxy clusters observed with the Chandra...