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相关论文: Cocoon shock, X-ray cavities and extended Inverse …

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The radio lobes of the radio galaxy Hercules A contain intriguing ring-like structures concentric with the jet axis. To investigate the occurrence of such features, we have used hydrodynamic simulations of jets with a range of Mach numbers…

天体物理学 · 物理学 2009-11-07 Curtis J. Saxton , Geoffrey V. Bicknell , Ralph S. Sutherland

We present the results from a 42 ks \chandra ACIS observation of the galaxy cluster A478. This cluster is generally considered to be highly relaxed. The \chandra image reveals, for the first time, X-ray cavities in the hot gas within the…

天体物理学 · 物理学 2009-09-17 M. Sun , C. Jones , S. S. Murray , S. W. Allen , A. C. Fabian , A. C. Edge

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

We present high angular resolution X-ray images and spectra from two {\em Chandra} ACIS-I observations of the X-ray jet in the nearby radio galaxy Centaurus A. We find that the X-ray emission from the jet is composed of a low surface…

天体物理学 · 物理学 2009-11-07 R. P. Kraft , W. R. Forman , C. Jones , S. S. Murray , M. J. Hardcastle , D. M. Worrall

The radio source Hercules A resides at the center of a cooling flow cluster of galaxies at redshift z = 0.154. A Chandra X-ray image reveals a shock front in the intracluster medium (ICM) surrounding the radio source, about 160 kpc from the…

天体物理学 · 物理学 2009-11-11 P. E. J. Nulsen , D. C. Hambrick , B. R. McNamara , D. Rafferty , L. Birzan , M. W. Wise , L. P. David

We report the discovery with Chandra of X-ray-emitting gas associated with the jet-cloud interaction in the radio galaxy 3C 277.3 (Coma A), a source that falls in the most important power range for radio-mode feedback in the Universe. This…

高能天体物理现象 · 物理学 2016-02-17 D. M. Worrall , M. Birkinshaw , A. J. Young

We report the first X-ray detection of a proto-supermassive binary black hole at the centre of Abell 400. Using the Chandra ACIS, we are able to clearly resolve the two active galactic nuclei in 3C 75, the well known double radio source at…

天体物理学 · 物理学 2009-11-11 Daniel S. Hudson , Thomas H. Reiprich , Tracy E. Clarke , Craig L. Sarazin

We examine a systematic comparison of jet-knots, hotspots and radio lobes recently observed with Chandra and ASCA. This report will discuss the origin of their X-ray emissions and investigate the dynamics of the jets. The data was compiled…

天体物理学 · 物理学 2009-11-10 Jun Kataoka , Lukasz Stawarz

Deep Chandra observations of the Hydra A Cluster reveal a feature in the X-ray surface brightness that surrounds the 330 MHz radio lobes of the AGN at the cluster center. Surface brightness profiles of this feature and its close association…

天体物理学 · 物理学 2008-11-26 P. E. J. Nulsen , B. R. McNamara , M. W. Wise , L. P. David

We use deep archival Chandra and XMM-Newton observations of three of the brightest cluster-centre radio galaxies in the sky, Cygnus A, Hercules A and Hydra A, to search for inverse-Compton emission from the population of electrons…

宇宙学与河外天体物理 · 物理学 2015-05-18 M. J. Hardcastle , J. H. Croston

This paper presents a comprehensive analysis of 30 ks Chandra and 46.8 ks (13 Hr) 1.4 GHz GMRT radio data on the cool-core cluster RXCJ0352.9+1941 with an objective to investigate AGN activities at its core. This study confirms a pair of…

高能天体物理现象 · 物理学 2024-09-04 Satish S. Sonkamble , S. K. Kadam , Surajit Paul , M. B. Pandge , P. K. Pawar , M. K. Patil

Cygnus A, the nearest truly powerful radio galaxy, resides at the centre of a massive galaxy cluster. Chandra X-ray observations reveal its cocoon shocks, radio lobe cavities and an X-ray jet, which are discussed here. It is argued that…

高能天体物理现象 · 物理学 2015-06-23 Paul E. J. Nulsen , Andrew J. Young , Ralph P. Kraft , Brian R. McNamara , Michael W. Wise

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…

天体物理学 · 物理学 2007-05-23 J. Siebert , N. Kawai , W. Brinkmann

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 new, high dynamic range VLA images of the inner jet of the closest radio galaxy, Centaurus A. Over a ten-year baseline we detect apparent sub-luminal motions (v ~ 0.5c) in the jet on scales of hundreds of pc. The inferred speeds…

天体物理学 · 物理学 2008-11-26 M. J. Hardcastle , D. M. Worrall , R. P. Kraft , W. R. Forman , C. Jones , S. S. Murray

We report the Chandra detection of an X-ray jet in 3C 15. The peak of the X-ray emission in the jet is 4.1'' (a projected distance of 5.1 kpc) from the nucleus, and coincident with a component previously identified in the radio and optical…

天体物理学 · 物理学 2009-11-10 J. Kataoka , J. P. Leahy , P. G. Edwards , M. Kino , F. Takahara , Y. Serino , N. Kawai , A. R. Martel

Centaurus A (Cen~A) is the nearest active radio galaxy, which has kiloparsec (kpc) scale jets and {giant lobes detected by various instruments in radio and X-ray frequency ranges}. The $Fermi$--Large Area Telescope and High Energy…

高能天体物理现象 · 物理学 2019-08-07 Kazuhisa Tanada , Jun Kataoka , Yoshiyuki Inoue

We analyse new Chandra observations of the nearest (D=4 Mpc) Seyfert 2 active galaxy, Circinus, and match them to pre-existing radio, infrared and optical data to study the kpc-scale emission. The proximity of Circinus allows us to observe…

宇宙学与河外天体物理 · 物理学 2012-10-09 Beatriz Mingo , Martin J. Hardcastle , Judith H. Croston , Daniel A. Evans , Preeti Kharb , Ralph P. Kraft , Emil Lenc

We present results from deeper {\em Chandra} observations of the southwest radio lobe of Centaurus A, first described by Kraft et al. (2003). We find that the sharp X-ray surface brightness discontinuity extends around $\sim$75% of the…

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
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