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Related papers: The dynamics of the giant radio galaxy 3C 457

200 papers

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…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-13 Ian Smail , B. D. Lehmer , R. J. Ivison , D. M. Alexander , R. G. Bower , J. A. Stevens , J. E. Geach , C. A. Scharf , K. E. K. Coppin , W. J. M. van Breugel , .

Inverse Compton (IC) scattering of nuclear photons with relativistic electrons in the lobes of powerful radio galaxies and quasars can give detectable extended X-ray emission from the radio lobes if relativistic electrons with a Lorentz…

Astrophysics · Physics 2009-11-06 G. Brunetti , M. Cappi , G. Setti , L. Feretti , D. E. Harris

We report the results of a Suzaku X-ray imaging study of NGC6251, a nearby giant radio galaxy with intermediate FR I/II radio properties. Our pointing direction was centered on the gamma -ray emission peak recently discovered with Fermi-LAT…

High Energy Astrophysical Phenomena · Physics 2015-06-04 Y. Takeuchi , J. Kataoka , L. Stawarz , Y. Takahashi , K. Maeda , T. Nakamori , C. C. Cheung , A. Celotti , Y. Tanaka , T. Takahashi

We present the results of the analysis of an archival 15 ks XMM-Newton observation of the nearby (z=0.057) radio-loud source 3C445, optically classified as a Broad-Line Radio Galaxy. While the RGS data are of insufficient quality to allow a…

Astrophysics · Physics 2009-06-23 R. M. Sambruna , J. N. Reeves , V. Braito

We report on deep Chandra X-ray Telescope imaging observations of 4C 63.20, one of the few known radio galaxies at z>3.5. The X-ray counterpart is resolved into a core plus two off-nuclear sources that (combined) account for close to 30% of…

High Energy Astrophysical Phenomena · Physics 2020-08-12 Kate Napier , Adi Foord , Elena Gallo , Gabriele Ghisellini , Edmund Hodges-Kluck , Jianfeng Wu , Francesco Haardt , Benedetta Ciardi

We present the analysis of five joint XMM-Newton/NuSTAR observations, 20 ks each and separated by 12 days, of the broad-line radio galaxy 3C 382. The data were obtained as part of a campaign performed in September-October 2016…

New Chandra observations of the giant (0.5 Mpc) radio galaxy 4C23.56 at z = 2.5 show X-rays in a linear structure aligned with its radio emission, but anti-correlated with the detailed radio structure. Consistent with the powerful, high-z…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-19 Katherine Blundell , Andy Fabian

We report the results from a {\it Chandra} observation of the powerful nearby (z=0.1744) radio galaxy 3C 219. We find evidence for non--thermal X-ray emission from the radio lobes which fits fairly well with a combination of IC scattering…

Astrophysics · Physics 2007-05-23 G. Brunetti , A. Comastri , D. Dallacasa , M. Bondi , M. Pedani , G. Setti

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…

Astrophysics · Physics 2009-11-07 C. A. Scharf , I. Smail , R. Ivison , R. G. Bower , W. van Breugel , M. Reuland

We present an investigation of the relationships between the radio properties of a giant radio galaxy MRC B0319-454 and the surrounding galaxy distribution with the aim of examining the influence of intergalactic gas and gravity associated…

Astrophysics · Physics 2009-11-13 V. Safouris , R. Subrahmanyan , G. V. Bicknell , L. Saripalli

The XMM-Newton observation of the nearby FR-II radio galaxy 3C 98 is reported. In two exposures on the target, faint diffuse X-ray emission associated with the radio lobes was significantly detected, together with a bright X-ray active…

Astrophysics · Physics 2009-11-13 N. Isobe , K. Makishima , M. Tashiro , S. Hong

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…

High Energy Astrophysical Phenomena · Physics 2014-11-20 Eric S. Perlman , Markos Georganopoulos , Emily M. May , Demosthenes Kazanas

The appearance of the jets and lobes of some radio galaxies makes it difficult to assign them to a known class of objects. This is often due to the activity of the central engine and/or interactions with the environment, as well as…

Astrophysics of Galaxies · Physics 2024-11-05 M. Weżgowiec , M. Jamrozy , K. T. Chyży , M. J. Hardcastle , A. Kuźmicz , G. Heald , T. W. Shimwell

We present the results of simultaneous XMM-Newton and RXTE observations of the Broad-Line Radio Galaxy 3C 111. We find that the Compton reflection bump is extremely weak, however, broad residuals are clearly present in the spectrum near the…

We present ROSAT PSPC observations of the twin-jet radio galaxy 3C449. The soft X-ray emission from this object is dominated by an extended halo with a scale comparable to that of the radio source. The asymmetry of the X-ray emission is…

Astrophysics · Physics 2009-10-30 M. J. Hardcastle , D. M. Worrall , M. Birkinshaw

We present the first broad-band X-ray study of the nuclei of 14 hard X-ray selected giant radio galaxies, based both on the literature and on the analysis of archival X-ray data from NuSTAR, XMM-Newton, Swift and INTEGRAL. The X-ray…

High Energy Astrophysical Phenomena · Physics 2018-09-26 F. Ursini , L. Bassani , F. Panessa , A. J. Bird , G. Bruni , M. Fiocchi , A. Malizia , L. Saripalli , P. Ubertini

The recent discovery of the gamma-ray emission from the lobes of the closest radio galaxy Centaurus A by Fermi implies the presence of high-energy electrons at least up to gamma ~ 10^5 - 10^6. These high-energy electrons are required to…

High Energy Astrophysical Phenomena · Physics 2015-05-27 F. Massaro , M. Ajello

We present the first high signal-to-noise XMM-Newton observations of the broad-line radio galaxy 3C 411. After fitting various spectral models, an absorbed double power-law continuum and a blurred relativistic disk reflection model (kdblur)…

High Energy Astrophysical Phenomena · Physics 2014-08-11 Allison Bostrom , Christopher S. Reynolds , Francesco Tombesi