Results 11 to 20 of about 254 (138)

Turbulent heating in galaxy clusters brightest in X-rays [PDF]

open access: yesNature, 2014
published in ...
I. Zhuravleva   +11 more
openaire   +11 more sources

X-RAY POINT SOURCES AND RADIO GALAXIES IN CLUSTERS OF GALAXIES [PDF]

open access: yesThe Astrophysical Journal, 2009
Using Chandra imaging spectroscopy and VLA L-band maps, we have identified radio galaxies at P(1.4 GHz) >= 3x10^{23} W Hz^{-1} and X-ray point sources (XPSs) at L(0.3-8 keV) >= 10^{42} ergs s^{-1} in 11 moderate redshift (0.2 99.999% level. All but one of the XPSs are hosted by luminous ellipticals which otherwise show no other evidence for AGN ...
Hart, Quyen N.   +2 more
openaire   +2 more sources

Baryons at the Edge of the X-ray–Brightest Galaxy Cluster [PDF]

open access: yesScience, 2011
The Suzaku satellite provides a census of the gas, metals, and dark matter out to the outskirts of the Perseus Cluster.
Simionescu, Aurora   +10 more
openaire   +3 more sources

Simulating the soft X-ray excess in clusters of galaxies [PDF]

open access: yesAstronomy & Astrophysics, 2005
The detection of excess of soft X-ray or Extreme Ultraviolet (EUV) radiation, above the thermal contribution from the hot intracluster medium (ICM), has been a controversial subject ever since the initial discovery of this phenomenon. We use a large--scale hydrodynamical simulation of a concordance $Λ$CDM model, to investigate the possible thermal ...
CHENG L. M.   +9 more
openaire   +4 more sources

X-ray clusters of galaxies as tracers of structure in the Universe [PDF]

open access: yesNature, 2001
27 pages, 7 figures, to appear as a Review in Nature, 4 January 2001 issue (higher resolution figures available at http://www.daut.univ.trieste.it/borgani/Nature/)
Borgani, S., Guzzo, L.
openaire   +3 more sources

The impact of galaxy formation on the X-ray evolution of clusters [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2001
We present a new model for the X-ray properties of the intracluster medium that explicitly includes heating of the gas by the energy released during the evolution of cluster galaxies. We calculate the evolution of clusters by combining the semi-analytic model of galaxy formation of Cole et al.
Bower, R. G.   +5 more
openaire   +4 more sources

X-ray Morphology of Clusters of Galaxies [PDF]

open access: yesHighlights of Astronomy, 1992
AbstractThe ROSAT observatory with its high spatial resolution X-ray telescope is an ideal instrument for the study of clusters of galaxies. In the first part of the mission an All Sky X-ray Survey was conducted with ROSAT. Here we present first results of observations of Virgo, Perseus and some other clusters of galaxies from the All Sky Survey. These
H. Böhringer   +4 more
openaire   +1 more source

Metallicity Gradients in X‐Ray Clusters of Galaxies

open access: yesThe Astrophysical Journal, 2001
8 pages, 5 figure, 2 tables.
De Grandi, Sabrina, Molendi, Silvano
openaire   +2 more sources

X-ray observations of Clusters of Galaxies

open access: yesProceedings of the International School of Physics “Enrico Fermi”, 2005
40 pages, 37 figures. Review article based on invited summer school lectures at "Background Microwave Radiation and Intracluster Cosmology", July 2004, Villa Monastero, Varenna, Italy. To appear in Proc. Enrico Fermi, International School of Physics Course CLIX, eds. F. Melchiorri & Y. Rephaeli.
openaire   +2 more sources

Primeval clusters of galaxies and the X-ray background [PDF]

open access: yesSymposium - International Astronomical Union, 1978
The X-ray telescope for HEAO-B, due for launch next year, will extend our observing power in X-ray astronomy by a very large factor. For example, its sensitivity to point sources will be 103 greater than the limit of existing X-ray sky surveys. Even more intriguing will be its capability to image the all-sky X-ray background radiation on an arc minute ...
openaire   +1 more source

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