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We present a systematic analysis of the extended X-ray emission discovered around 35 FR II radio galaxies from the revised Third Cambridge catalog (3CR) Chandra Snapshot Survey with redshifts between 0.05 to 0.9. We aimed to (i) test for…

This paper studied the faint, diffuse extended X-ray emission associated with the radio lobes and the hot gas in the intracluster medium (ICM) environment for a sample of radio galaxies. We used shallow ($\sim 10$ ks) archival Chandra…

We present Chandra observations of two relatively high redshift FRII radio galaxies, 3C 432 and 3C 191 (z=1.785 and z=1.956 respectively), both of which show extended X-ray emission along the axis of the radio jet or lobe. This X-ray…

天体物理学 · 物理学 2009-09-17 M. C. Erlund , A. C. Fabian , Katherine M. Blundell , A. Celotti , C. S. Crawford

We present sensitive, high-resolution, X-ray imaging from Chandra of the high-redshift radio galaxy 4C 41.17 (z=3.8). Our 150-ks Chandra exposure detects strong X-ray emission from a point source coincident with the nucleus of the radio…

天体物理学 · 物理学 2009-11-07 C. A. Scharf , I. Smail , R. Ivison , R. G. Bower , W. van Breugel , M. Reuland

X-ray selected galaxy group samples are usually generated by searching for extended X- ray sources that reflect the thermal radiation of the intragroup medium. On the other hand, large radio galaxies that regularly occupy galaxy groups also…

We present results from a 49.4 ks Chandra/ACIS-S observation of the nearby ($z$=0.059) X-shaped FRII radio galaxy 3C~403. This is the first Chandra observation of an X-shaped radio galaxy, and one of the goals of this pioneering study is to…

天体物理学 · 物理学 2009-11-10 R. P. Kraft , M. J. Hardcastle , D. M. Worrall , S. S. Murray

Most old distant radio galaxies should be extended X-ray sources due to inverse Compton scattering of Cosmic Microwave Background (CMB) photons. Such sources can be an important component in X-ray surveys for high redshift clusters, due to…

天体物理学 · 物理学 2016-08-30 A. Celotti , A. C. Fabian

Spectral analysis of ROSAT PSPC and ASCA archive data and a recent ROSAT HRI observation of the powerful FRII radio galaxy 3C 219 reveal an absorbed point-like source, coincident with the nucleus, and a non-thermal extended component…

天体物理学 · 物理学 2007-05-23 G. Brunetti , A. Comastri , G. Setti , L. Feretti

Recent observations of high energy (> 20 keV) X-ray emission in a few clusters of galaxies broaden our knowledge of physical phenomena in the intracluster space. This emission is likely to be nonthermal, probably resulting from Compton…

天体物理学 · 物理学 2009-11-13 Y. Rephaeli , J. Nevalainen , T. Ohashi , A. M. Bykov

We report on the detection of a soft spatially-extended component of X-ray emission around four intermediate-redshift 3C quasars observed with Chandra: 3C254, 3C263, 3C275.1 and 3C281. The bolometric luminosity of this emission ranges over…

天体物理学 · 物理学 2009-09-17 C. S. Crawford , A. C. Fabian

We report on the {\it Chandra} discovery of large scale non--thermal emission features in the double lobed SSRL quasar 3C 207 (z=0.684). These are: a diffuse emission well correlated with the western radio lobe, a bright one sided jet whose…

天体物理学 · 物理学 2009-11-07 G. Brunetti , M. Bondi , A. Comastri , G. Setti

We present new {\it Chandra} observations of the radio galaxy 3C 445, centered on its southern radio hotspot. Our observations detect X-ray emission displaced upstream and to the west of the radio-optical hotspot. Attempting to reproduce…

高能天体物理现象 · 物理学 2014-11-20 Eric S. Perlman , Markos Georganopoulos , Emily M. May , Demosthenes Kazanas

An 80 ksec Chandra ACIS observation of the radio galaxy 3C 452 is reported. A diffuse X-ray emission associated with the lobes has been detected with high statistical significance, together with the X-ray nucleus of the host galaxy. The…

天体物理学 · 物理学 2009-11-07 N. Isobe , M. Tashiro , K. Makishima , N. Iyomoto , M. Suzuki , M. M. Murakami , M. Mori , K. Abe

We describe new Chandra spectroscopy data of the cluster which harbors the prototypical "head tail" radio galaxy 3C 129 and the weaker radio galaxy 3C 129.1. We combined the Chandra data with Very Large Array (VLA) radio data taken at 0.33,…

天体物理学 · 物理学 2009-11-07 H. Krawczynski , D. E. Harris , R. Grossman , W. Lane , N. Kassim , A. G. Willis

This paper presents the analysis of Chandra X-ray snapshot observations of a subsample of the extragalactic sources listed in the revised Third Cambridge radio catalog (3CR), previously lacking X-ray observations and thus observed during…

We present Chandra X-ray observations of the powerful radio galaxy 3C171, which reveal an extended region of X-ray emission spatially associated with the well-known 10-kpc scale optical emission-line region around the radio jets. We argue…

宇宙学与河外天体物理 · 物理学 2015-05-14 M. J. Hardcastle , F. Massaro , D. E. Harris

We analyse a 100-ks Chandra observation of the powerful radio galaxy, 4C60.07 at z=3.79. We identify extended X-ray emission with Lx~10^45 erg/s across a ~90-kpc region around the radio galaxy. The energetics of this X-ray halo and its…

We investigated the X-ray emission properties of the powerful radio galaxy 3C 459 revealed by a recent Chandra follow-up observation carried out in October 2014 with a 62 ks exposure. We performed an X-ray spectral analysis from a few…

高能天体物理现象 · 物理学 2018-12-12 A. Maselli , R. P. Kraft , F. Massaro , M. J. Hardcastle

We present multi-frequency radio observations with the Giant Metrewave Radio Telescope and Very Large Array, and X-ray observations with the X-ray Multi-Mirror Mission ({\it XMM-Newton}) telescope of the giant radio source (GRS) 3C 457. We…

宇宙学与河外天体物理 · 物理学 2015-05-13 C. Konar , M. J. Hardcastle , J. H. Croston , D. J. Saikia

We report results from XMM-Newton and Chandra observations of the nearby (z = 0.067) giant radio galaxy 3C 35. We find evidence for an X-ray emitting gas belt, orthogonal to and lying between the lobes of 3C 35, which we interpret as…

宇宙学与河外天体物理 · 物理学 2013-02-28 Elizabeth J. A. Mannering , Diana M. Worrall , Mark Birkinshaw
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