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Using the X-ray data from \ASCA, spectral and spatial properties of the intra-cluster medium (ICM) of the cD cluster Abell 1795 are studied, up to a radial distance of $\sim 12'$ ($\sim 1.3$ $h_{50}^{-1}$ kpc). The ICM temperature and…

Astrophysics · Physics 2009-10-30 H. Xu , K. Makishima , Y. Fukazawa , Y. Ikebe , K. Kikuchi , T. Ohashi , T. Tamura

We present new X-ray (Chandra) and radio (ATCA) observations of the z=0.09 radio galaxy PKS B1416-493, a member of the southern equivalent of the 3CRR sample. We find the source to be embedded in a previously unrecognized bright kT=4.6 keV…

High Energy Astrophysical Phenomena · Physics 2017-03-22 D. M. Worrall , M. Birkinshaw

We present results from an analysis of a Chandra observation of the cluster of galaxies Abell 3581. We discover the presence of a point-source in the central dominant galaxy which is coincident with the core of the radio source PKS…

Astrophysics · Physics 2009-09-17 R. M. Johnstone , A. C. Fabian , R. G. Morris , G. B. Taylor

We present a study of the cavity system in the galaxy cluster RBS 797 based on Chandra and VLA data. RBS 797 (z = 0.35), is one of the most distant galaxy clusters in which two pronounced X-ray cavities have been discovered. The Chandra…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-04 Alberto Doria , Myriam Gitti , Stefano Ettori , Fabrizio Brighenti , Paul E. J. Nulsen , Brian R. McNamara

The radio galaxy 1321+045 is a rare example of a young, compact steep spectrum source located in the center of a z=0.263 galaxy cluster. Using a combination of Chandra, VLBA, VLA, MERLIN and IRAM 30m observations, we investigate the…

The X-ray emission in many clusters of galaxies shows a central peak in surface brightness coincident with a drop in temperature. These characterize a cooling flow. There is often a radio source also at the centre of such regions. Data from…

Astrophysics · Physics 2007-05-23 A. C. Fabian

We present results from a deep (174 ks) Chandra observation of the FR-II radio galaxy 3C 220.1, the central brightest cluster galaxy (BCG) of a $kT \sim$ 4 keV cluster at $z=0.61$. The temperature of the hot cluster medium drops from…

High Energy Astrophysical Phenomena · Physics 2020-01-22 Wenhao Liu , Ming Sun , Paul E. J. Nulsen , Diana M. Worrall , Mark Birkinshaw , Craig Sarazin , William R. Forman , Christine Jones , Chong Ge

We present results from an analysis of two Chandra observations of the rich, nearby galaxy cluster Abell 2199. We find evidence (having corrected for projection effects) for radial gradients in temperature and metallicity in the X-ray…

Astrophysics · Physics 2009-09-17 R. M. Johnstone , S. W. Allen , A. C. Fabian , J. S. Sanders

We present a Chandra observation of the candidate BL Lac object EXO 0423.4-0840. The X-ray emission from EXO 0423.4-0840 is clearly extended, and is associated with an optical early-type galaxy, MCG-01-12-005, at the centre of cluster ClG…

Astrophysics · Physics 2009-11-10 Elena Belsole , Mark Birkinshaw , Diana M. Worrall

We present a weak-lensing analysis of the galaxy cluster CL J1226+3332 at z=0.89 using Hubble Space Telescope Advanced Camera for Surveys images. The cluster is the hottest (>10 keV), most X-ray luminous system at z>0.6 known to date. The…

Astrophysics · Physics 2011-02-11 M. J. Jee , J. A. Tyson

We report the detection of both soft and hard excess X-ray emission in the cluster of galaxies A 2199, based upon spatially resolved spectroscopy with data from the BeppoSAX, EUVE and ROSAT missions. The excess emission is visible at radii…

We report the discovery of a pair of giant cavities, each nearly 200 kpc in diameter, embedded in the gaseous halo of the redshift z=0.216 galaxy cluster MS0735.6+7421. The cavities appear as surface brightness depressions in an image of…

We investigate the X-ray properties of the powerful radio galaxy Hercules A (3C 348) using ROSAT HRI, PSPC and ASCA observations. The ASCA data are well fit by a thermal plasma model with a temperature of about 4.3 keV and abundances 0.4…

Astrophysics · Physics 2007-05-23 J. Siebert , N. Kawai , W. Brinkmann

We present a multiwavelength study of RXC J2014.8-2430, the most extreme cool-core cluster in the Representative $XMM-Newton$ Cluster Structure Survey (REXCESS), using $Chandra$ X-ray, Southern Astrophysical Research (SOAR) Telescope,…

(abridged) We report results from a Chandra study of the central regions of the nearby, X-ray bright, Ophiuchus Cluster (z = 0.03), the second-brightest cluster in the sky. Our study reveals a dramatic, close-up view of the stripping and…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-14 E. T. Million , S. W. Allen , N. Werner , G. B. Taylor

The cooling flow cluster Hydra A was observed during the orbital activation and calibration phase of the Chandra Observatory. While the X-ray image of the cluster exhibits complex structure in the central region as reported in McNamara…

Astrophysics · Physics 2008-11-26 L. P. David , P. E. J. Nulsen , B. R. McNamara , W. Forman , C. Jones , T. Ponman , B. Robertson , M. Wise

The physics of the coolest phases in the hot Intra-Cluster Medium (ICM) of clusters of galaxies is yet to be fully unveiled. X-ray cavities blown by the central Active Galactic Nucleus (AGN) contain enough energy to heat the surrounding gas…

Cosmology and Nongalactic Astrophysics · Physics 2011-05-25 J. de Plaa , N. Werner , A. Simionescu , J. S. Kaastra , Y. G. Grange , Jacco Vink

We have analyzed X-ray spectra from six galaxy clusters which contain cooling flows: A85, A478, A1795, A2142, A2147, & A2199. The X-ray spectra were taken with the HEAO1-A2 Medium and High Energy Detectors and the Einstein Solid State…

Astrophysics · Physics 2009-10-28 Mark J. Henriksen , Raymond E. White

The initial results from XMM-Newton observations of the rich cluster of galaxies Abell 1795 are presented. The spatially-resolved X-ray spectra taken by the European Photon Imaging Cameras (EPIC) show a temperature drop at a radius of $\sim…

We present results from a 35 ks {\em Chandra}/ACIS-I observation of the hot ICM around the FR II radio galaxy 3C 388. 3C 388 resides in a cluster environment with an ICM temperature of $\sim$3.5 keV. We detect cavities in the ICM coincident…

Astrophysics · Physics 2009-11-13 R. P. Kraft , J. Azcona , W. R. Forman , M. J. Hardcastle , C. Jones , S. S. Murray