Heating hot atmospheres with active galactic nuclei
BR McNamara, PEJ Nulsen - Annu. Rev. Astron. Astrophys., 2007 - annualreviews.org
High resolution X-ray spectroscopy of the hot gas in galaxy clusters has shown that the gas
is not cooling to low temperatures at the predicted rates of hundreds to thousands of solar …
is not cooling to low temperatures at the predicted rates of hundreds to thousands of solar …
Chern–Simons modified general relativity
S Alexander, N Yunes - Physics Reports, 2009 - Elsevier
Chern–Simons modified gravity is an effective extension of general relativity that captures
leading-order, gravitational parity violation. Such an effective theory is motivated by anomaly …
leading-order, gravitational parity violation. Such an effective theory is motivated by anomaly …
Cosmological hydrodynamics with adaptive mesh refinement-a new high resolution code called ramses
R Teyssier - Astronomy & Astrophysics, 2002 - aanda.org
A new N-body and hydrodynamical code, called RAMSES, is presented. It has been
designed to study structure formation in the universe with high spatial resolution. The code is …
designed to study structure formation in the universe with high spatial resolution. The code is …
Chandra sample of nearby relaxed galaxy clusters: mass, gas fraction, and mass-temperature relation
We present gas and total mass profiles for 13 low-redshift, relaxed clusters spanning a
temperature range 0.7-9 keV, derived from all available Chandra data of sufficient quality. In …
temperature range 0.7-9 keV, derived from all available Chandra data of sufficient quality. In …
Cosmological parameters from observations of galaxy clusters
Studies of galaxy clusters have proved crucial in helping to establish the standard model of
cosmology, with a Universe dominated by dark matter and dark energy. A theoretical basis …
cosmology, with a Universe dominated by dark matter and dark energy. A theoretical basis …
Dark light, dark matter, and the misalignment mechanism
We explore the possibility that the dark matter is a condensate of a very light vector boson.
Such a condensate could be produced during inflation, provided the vector mass arises via …
Such a condensate could be produced during inflation, provided the vector mass arises via …
Tracing cosmic evolution with clusters of galaxies
GM Voit - Reviews of Modern Physics, 2005 - APS
The most successful cosmological models to date envision structure formation as a
hierarchical process in which gravity is constantly drawing lumps of matter together to form …
hierarchical process in which gravity is constantly drawing lumps of matter together to form …
The mass function of an X-ray flux-limited sample of galaxy clusters
TH Reiprich, H Boehringer - The Astrophysical Journal, 2002 - iopscience.iop.org
ABSTRACT A new X-ray–selected and X-ray flux–limited galaxy cluster sample is
presented. Based on the ROSAT All-Sky Survey, the 63 brightest clusters with galactic …
presented. Based on the ROSAT All-Sky Survey, the 63 brightest clusters with galactic …
Chandra cluster cosmology project. II. Samples and X-ray data reduction
We discuss the measurements of the galaxy cluster mass functions at z≈ 0.05 and z≈ 0.5
using high-quality Chandra observations of samples derived from the ROSAT PSPC All-Sky …
using high-quality Chandra observations of samples derived from the ROSAT PSPC All-Sky …
What is a cool-core cluster? a detailed analysis of the cores of the X-ray flux-limited HIFLUGCS cluster sample
We use the largest complete sample of 64 galaxy clusters (HIghest X-ray FLUx Galaxy
Cluster Sample) with available high-quality X-ray data from Chandra, and apply 16 cool …
Cluster Sample) with available high-quality X-ray data from Chandra, and apply 16 cool …