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相关论文: Powerful yet lonely: Is 3C 297 a high-redshift fos…

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Gemini Multi Object Spectrograph medium-resolution spectra and photometric data of 39 objects in the field of the radio galaxy 3C 17 are presented. Based on the new data, a previously uncataloged cluster of galaxies is identified at a mean…

We present the results of XMM-Newton observations of three high-redshift powerful radio galaxies 3C 184, 3C 292 and 3C 322. Although none of the sources lies in as rich an X-ray-emitting environment as is seen for some powerful radio…

天体物理学 · 物理学 2007-05-23 E. Belsole , D. M. Worrall , M. J. Hardcastle , M. Birkinshaw , C. R. Lawrence

We present results on the physical states of three high-redshift powerful radio galaxies (3C 292 at z=0.7, 3C 184 at z=1, and 3C322 at z=1.7). They were obtained by combining radio measurements with X-ray measurements from XMM-Newton that…

天体物理学 · 物理学 2009-11-10 E. Belsole , D. M. Worrall , M. J. Hardcastle

We present a multi-wavelength analysis based on archival radio, optical and X-ray data of the complex radio source 3C 196.1, whose host is the brightest cluster galaxy of a $z=0.198$ cluster. HST data show H$\alpha$+[N II] emission aligned…

高能天体物理现象 · 物理学 2018-11-07 F. Ricci , L. Lovisari , R. P. Kraft , F. Massaro , A. Paggi , E. Liuzzo , G. Tremblay , W. R. Forman , S. Baum , C. O'Dea , B. Wilkes

Context. High redshift radio galaxies are among the most massive galaxies at their redshift, are often found at the center of protoclusters of galaxies, and are expected to evolve into the present day massive central cluster galaxies. Thus…

This paper contains an analysis of short Chandra observations of 19 3C sources with redshifts between 0.3 and 0.5 not previously observed in the X-rays. This sample is part of a project to obtain Chandra data for all of the extragalactic…

高能天体物理现象 · 物理学 2015-06-15 F. Massaro , D. E. Harris , G. Tremblay , E. Liuzzo , A. Bonafede , A. Paggi

We present a Chandra observation of the powerful radio galaxy 3C294 showing clear evidence for a surrounding intracluster medium. At a redshift of 1.786 this is the most distant cluster of galaxies yet detected in X-rays. The radio core is…

天体物理学 · 物理学 2009-11-06 A. C. Fabian , C. S. Crawford , S. Ettori , J. S. Sanders

We report on the very first radio detection associated with the peculiar hourglass-morphology X-rays surrounding 3C 294 at z=1.8. Using International Low Frequency Array (LOFAR) data at 144 MHz and Chandra data at 0.3-6 keV, we find that…

星系天体物理 · 物理学 2025-12-19 Vijay H. Mahatma , Andrew C. Fabian , Leah K. Morabito

We report the results from a 200 ks Chandra observation of the z=1.786 radio galaxy 3C294 and its cluster environment, increasing by tenfold our earlier observation. The diffuse emission, extending about 100 kpc around the nucleus, has a…

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

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

We investigate the properties of the environment around 20 powerful radio galaxies and quasars at redshifts between 0.45 and 1. Using XMM-Newton and Chandra observations we probe the spatial distribution and the temperature of the cluster…

天体物理学 · 物理学 2009-11-13 Elena Belsole , Diana M. Worrall , Martin J. Hardcastle , Judith H. Croston

We present a study of quasar host galaxy 3C 297 which is home to a powerful bent-jet radio source suggesting vigorous interaction with a dense ISM and/or jet precession. Archival HST imaging showed interestingly perturbed morphology of the…

Non-thermal properties of galaxy clusters have been studied with detailed and deep radio images in comparison with X-ray data. While much progress has been made, most of the studied clusters are at a relatively low redshift (z < 0.3). We…

宇宙学与河外天体物理 · 物理学 2020-08-26 G. Giovannini , M. Cau , A. Bonafede , H. Ebeling , L. Feretti , M. Girardi , M. Gitti , F. Govoni , A. Ignesti , M. Murgia , G. B. Taylor , V. Vacca

We present an analysis of archival Chandra data of the merging galaxy cluster ClG 0217+70. The Fe XXV He$\alpha$ X-ray emission line is clearly visible in the 25 ks observation, allowing a precise determination of the redshift of the…

高能天体物理现象 · 物理学 2020-10-07 X. Zhang , A. Simionescu , J. S. Kaastra , H. Akamatsu , D. N. Hoang , C. Stuardi , R. J. van Weeren , L. Rudnick , R. P. Kraft , S. Brown

We report the identification of a cluster of galaxies around the high-redshift radio galaxy 3CR184 at z = 0.996. The identification is supported by an excess of galaxies observed in projection in I band images (both in ground-based and HST…

天体物理学 · 物理学 2009-10-30 J. -M. Deltorn , O. Le Fevre , David Crampton , M. Dickinson

Using a combination of near-infrared and optical photometry, along with multi-object spectroscopy, we have confirmed the existence of a high-redshift cluster of galxies at z = 0.96. The cluster was found using a wide-angle tailed radio…

We discuss the properties of galaxies around the radio galaxy 3C 324 at z=1.2 based on BVRIK' multi-band imaging data. We have applied a photometric-redshift technique to objects in the 3C 324 field, and identified 35 objects as plausible…

We present the results of the dynamical analysis of the rich, hot, and X-ray very luminous galaxy cluster A2219, containing a powerful diffuse radio-halo. Our analysis is based on new redshift data for 27 galaxies in the cluster region,…

天体物理学 · 物理学 2009-11-10 W. Boschin , M. Girardi , R. Barrena Delgado , A. Biviano , L. Feretti , M. Ramella

We report the discovery of a giant radio halo in the galaxy cluster RXC J1514.9-1523 at z=0.22 with a relatively low X-ray luminosity, $L_{X \, [0.1-2.4 \rm \, kev]} \sim 7 \times 10^{44}$ erg s$^{-1}$. This faint, diffuse radio source is…

Chandra X-ray Observatory observations of the powerful, peculiar radio galaxy 3C123 have resulted in an X-ray detection of the bright eastern hotspot, with a 1-keV flux density of ~ 5 nJy. The X-ray flux and spectrum of the hotspot are…

天体物理学 · 物理学 2009-11-06 M. J. Hardcastle , M. Birkinshaw , D. M. Worrall
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