[HTML][HTML] Cooling flows in clusters of galaxies
AC Fabian - Annual Review of Astronomy and Astrophysics …, 1994 - adsabs.harvard.edu
Cooling Flows in Clusters of Galaxies ADS Classic is now deprecated. It will be completely
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retired in October 2019. This page will automatically redirect to the new ADS interface at that …
Cosmology with the Sunyaev-Zel'dovich effect
JE Carlstrom, GP Holder… - Annual Review of …, 2002 - annualreviews.org
▪ Abstract The Sunyaev-Zel'dovich effect (SZE) provides a unique way to map the large-
scale structure of the universe as traced by massive clusters of galaxies. As a spectral …
scale structure of the universe as traced by massive clusters of galaxies. As a spectral …
An overview of the performance and scientific results from the Chandra X‐Ray Observatory
MC Weisskopf, B Brinkman, C Canizares… - Publications of the …, 2002 - iopscience.iop.org
ABSTRACT The Chandra X‐Ray Observatory (CXO), the X‐ray component of NASA's Great
Observatories, was launched on 1999 July 23 by the space shuttle Columbia. After satellite …
Observatories, was launched on 1999 July 23 by the space shuttle Columbia. After satellite …
A textbook example of a bow shock in the merging galaxy cluster 1E 0657–56
M Markevitch, AH Gonzalez, L David… - The Astrophysical …, 2002 - iopscience.iop.org
The Chandra image of the merging, hot galaxy cluster 1E 0657-56 reveals a bow shock
propagating in front of a bullet-like gas cloud just exiting the disrupted cluster core. This is …
propagating in front of a bullet-like gas cloud just exiting the disrupted cluster core. This is …
X-ray spectroscopy of cooling clusters
JR Peterson, AC Fabian - Physics reports, 2006 - Elsevier
We review the X-ray spectra of the cores of clusters of galaxies. Recent high resolution X-ray
spectroscopic observations have demonstrated a severe deficit of emission at the lowest X …
spectroscopic observations have demonstrated a severe deficit of emission at the lowest X …
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 …
Magnetic fields in clusters of galaxies
F Govoni, L Feretti - International Journal of Modern Physics D, 2004 - World Scientific
The existence of magnetic fields associated with the intracluster medium in clusters of
galaxies is now well established through different methods of analysis. Magnetic fields are …
galaxies is now well established through different methods of analysis. Magnetic fields are …
A very deep Chandra observation of the Perseus cluster: shocks, ripples and conduction
We present the first results from a very deep Chandra X-ray observation of the core of the
Perseus cluster of galaxies. A pressure map reveals a clear thick band of high pressure …
Perseus cluster of galaxies. A pressure map reveals a clear thick band of high pressure …
Shocks and cold fronts in galaxy clusters
M Markevitch, A Vikhlinin - Physics Reports, 2007 - Elsevier
The currently operating X-ray imaging observatories provide us with an exquisitely detailed
view of the Megaparsec-scale plasma atmospheres in nearby galaxy clusters. At z< 0.05, the …
view of the Megaparsec-scale plasma atmospheres in nearby galaxy clusters. At z< 0.05, the …
A deep Chandra observation of the Perseus cluster: shocks and ripples
We present preliminary results from a deep observation lasting almost 200 ks of the centre of
the Perseus cluster of galaxies around NGC 1275. The X-ray surface brightness of the …
the Perseus cluster of galaxies around NGC 1275. The X-ray surface brightness of the …