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相关论文: Chandra and XMM-Newton Observations of NGC 6251

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During the course of an investigation on the interaction of the radio galaxy 3C129 and its ambient cluster gas, we found excess X-ray emission aligned with the northern radio jet. The emission extends from the weak X-ray core of the host…

天体物理学 · 物理学 2009-11-07 D. E. Harris , H. Krawczynski , G. B. Taylor

We report X-ray imaging of the powerful FR-II radio galaxy 3C353 using the Chandra X-ray Observatory. 3C353's two 4"-wide and 2'-long jets allow us to study in detail the internal structure of the large-scale relativistic outflows at both…

We present the first results from an X-ray and optical survey of a sample of AGN radio jets with Chandra and HST. We focus here on the first six sources observed at X-rays, in four of which a bright X-ray jet was detected for the first…

We have made a 30 ksec Chandra observation of the redshift z=0.63 GPS quasar B2 0738+313. We detected X-ray emission from the core and have discovered a 200 kpc (projected on the sky) X-ray jet. The X-ray jet is narrow and curves, following…

We report X-ray observations of the nearby, powerful radio galaxy Pictor A with the Chandra Observatory and optical and near uv observations of its western radio hot spot with the Hubble Space Telescope. X-ray emission is detected from the…

天体物理学 · 物理学 2009-10-31 A. S. Wilson , A. J. Young , P. L. Shopbell

Our Chandra observation of the FRI radio galaxy 3C66B has resulted in the first detection of an X-ray counterpart to the previously known radio, infra-red and optical jet. The X-ray jet is detected up to 7 arcsec from the core and has a…

天体物理学 · 物理学 2016-01-13 M. J. Hardcastle , M. Birkinshaw , D. M. Worrall

NGC 6251 is a luminous radio galaxy ~104 Mpc away that was detected significantly with the Fermi Gamma-ray Space Telescope, and before that with EGRET (onboard the Compton Gamma-ray Observatory). Different observational constraints favor a…

宇宙学与河外天体物理 · 物理学 2015-05-28 G. Migliori , P. Grandi , E. Torresi , C. Dermer , J. Finke , A. Celotti , R. Mukherjee , M. Errando , F. Gargano , F. Giordano , M. Giroletti

We have observed the twin-jet radio galaxy 3C296 with Chandra. X-ray emission is detected from the nucleus, from the inner parts of the radio jet, and from a small-scale thermal environment around the jet deceleration region. As we have…

天体物理学 · 物理学 2009-11-10 M. J. Hardcastle , D. M. Worrall , M. Birkinshaw , R. A. Laing , A. H. Bridle

We present spectral results, from Chandra and XMM-Newton observations, of a sample of 22 low-redshift (z < 0.1) radio galaxies, and consider whether the core emission originates from the base of a relativistic jet, an accretion flow, or…

天体物理学 · 物理学 2009-11-13 D. A. Evans , D. M. Worrall , M. J. Hardcastle , R. P. Kraft , M. Birkinshaw

The core-dominated radio-loud quasar PKS 0637-752 (z = 0.654) was the first celestial object observed with the Chandra X-ray Observatory, offering the early surprise of the detection of a remarkable X-ray jet. Several observations with a…

A puzzling feature of the {\it Chandra}--detected quasar jets is that their X-ray emission decreases faster along the jet than their radio emission, resulting to an outward increasing radio to X-ray ratio. In some sources this behavior is…

天体物理学 · 物理学 2016-08-30 Markos Georganopoulos , Demosthenes Kazanas

The radio source 3C 270, hosted by NGC 4261, is the brightest known example of counterjet X-ray emission from a low-power radio galaxy. We report on the X-ray emission of the jet and counterjet from 130 ks of Chandra data. We argue that the…

宇宙学与河外天体物理 · 物理学 2015-05-19 D. M. Worrall , M. Birkinshaw , E. O'Sullivan , A. Zezas , A. Wolter , G. Trinchieri , G. Fabbiano

This paper reports on a partially simultaneous observation of the bright Seyfert 1 Galaxy Mrk590, performed by XMM-Newton and Chandra. The long exposure (~100 ks) allows to investigate with great detail the Fe K complex at 6-7 keV and the…

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 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

The high spatial resolution of the Chandra X-ray Observatory allows us to study the environment of GPS/CSS sources to within an arcsec of the strong compact core. We present the discovery of X-ray jets in two GPS quasars, PKS1127-145 and B2…

We report the detection at X-rays of the radio/optical jet of 3C 371, from a short (10 ks) Chandra exposure in March 2000. We also present a new MERLIN observation at 1.4 GHz together with a renalysis of the archival HST WFPC2 F555W image.…

天体物理学 · 物理学 2009-11-06 Joseph E. Pesce , Rita M. Sambruna , F. Tavecchio , L. Maraschi , C. C. Cheung , C. Megan Urry , R. Scarpa

The Chandra X-ray observatory has proven to be a vital tool for studying high-energy emission processes in jets associated with Active Galactic Nuclei (AGN).We have compiled a sample of 27 AGN selected from the radio flux-limited MOJAVE…

高能天体物理现象 · 物理学 2015-05-27 Brandon Hogan , Matthew Lister , Preeti Kharb , Herman Marshall , Nathan Cooper

We report high resolution imaging of the nucleus of the Seyfert 1 galaxy NGC 4151 obtained with a 50 ks Chandra HRC observation. The HRC image resolves the emission on spatial scales of 0.5", ~30 pc, showing an extended X-ray morphology…

星系天体物理 · 物理学 2014-11-20 Junfeng Wang , G. Fabbiano , M. Karovska , M. Elvis , G. Risaliti , A. Zezas , C. G. Mundell

We report the first detection, with Chandra, of X-ray emission from the jet of the powerful narrow-line radio galaxy 3C 346. X-rays are detected from the bright radio and optical knot at which the jet apparently bends by about 70 degrees.…

天体物理学 · 物理学 2009-11-10 D. M. Worrall , M. Birkinshaw