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相关论文: Radio lobes and X-ray hot spots in the microquasar…

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We have studied the newly-discovered microquasar in NGC 7793 in radio, optical and X-ray bands. This system comprises a large (250 x 120 pc) line-emitting optical nebula, detected in H-alpha and HeII 4686. The optical nebula coincides with…

高能天体物理现象 · 物理学 2015-05-14 Roberto Soria , Manfred Pakull , Jess Broderick , Stephane Corbel , Christian Motch

We present results from {\em Chandra}/ACIS-S, {\em Spitzer}, {\em XMM-Newton}, {\em HST}, and VLA observations of the radio hot spots, extended environment, and nucleus of the nearby ($z$=0.0597) FR II radio galaxy 3C 33. This is a…

天体物理学 · 物理学 2011-02-11 R. P. Kraft , M. Birkinshaw , M. J. Hardcastle , D. A. Evans , J. H. Croston , D. M. Worrall , S. S. Murray

We present a detailed analysis of the XMM-Newton and Chandra observations of Abell 2626 focused on the X-ray and radio interactions. Within the region of the radio mini-halo (~70 kpc), there are substructures which are probably produced by…

天体物理学 · 物理学 2009-11-13 Ka-Wah Wong , Craig L. Sarazin , Elizabeth L. Blanton , Thomas H. Reiprich

NGC 7793 - S26 is an extended source (350 pc $\times$ 185 pc) previously studied in the radio, optical and x-ray domains. It has been identified as a micro-quasar which has inflated a super bubble. We used Integral Field Spectra from the…

高能天体物理现象 · 物理学 2015-06-11 M. A. Dopita , J. L. Payne , M. D. Filipović , T. G. Pannuti

We present the discovery of a powerful candidate microquasar in NGC 300, associated with the S 10 optical nebula (previously classified as a supernova remnant). Chandra images show four discrete X-ray knots aligned in the plane of the sky…

We report Chandra X-ray Observatory and 1.4 GHz Australian Long Baseline Array (LBA) observations of the radio galaxy PKS 2153--69 and its environment. The Chandra image reveals a roughly spherical halo of hot gas extending out to 30 kpc…

天体物理学 · 物理学 2009-11-10 A. J. Young , A. S. Wilson , S. J. Tingay , S. Heinz

We present the results of high resolution VLBI observations at 1.6 and 4.9 GHz of the radio-loud Seyfert galaxy, Mrk 6. These observations are able to detect a compact radio core in this galaxy for the first time. The core has an inverted…

星系天体物理 · 物理学 2015-06-18 P. Kharb , C. P. O'Dea , S. A. Baum , M. J. Hardcastle , D. Dicken , J. H. Croston , B. Mingo , J. Noel-Storr

We present a deep high-resolution Chandra X-ray Observatory image data of a powerful compact radio source PKS 0023-26 associated with a quasar at redshift 0.322. The earlier studies of the optical environment suggested that the source could…

星系天体物理 · 物理学 2025-08-01 A. Siemiginowska , R. Morganti , G. Fabbiano , E. O'Sullivan , T. Oosterloo , C. Tadhunter , D. Burke

We present the results of 20 ksec Chandra observations for each of 5 radio galaxies in the redshift range 2.0 < z < 2.6. For 4 of the 5 targets we detect unresolved X-ray components coincident with the radio nuclei. From spectral analysis…

天体物理学 · 物理学 2016-12-28 R. A. Overzier , D. E. Harris , C. L. Carilli , L. Pentericci , H. J. A. Rottgering , G. K. Miley

Here we present detailed analysis of the distinct X-ray emission features present within the Eastern radio lobe of the Pictor A galaxy, around the jet termination region, utilising the data obtained from the Chandra X-ray Observatory.…

高能天体物理现象 · 物理学 2021-11-02 R. Thimmappa , Ł. Stawarz , U. Pajdosz-Śmierciak , K. Balasubramaniam , V. Marchenko

We present a detailed spectral and spatial analysis of the X-ray properties of the compact and unusual radio galaxy 3C 346, combining information from ROSAT and ASCA. The dominant component of X-ray emission (~ 10^44 ergs/s in each of the…

天体物理学 · 物理学 2009-10-31 D. M. Worrall , M. Birkinshaw

We present results from two {\em Chandra}/ACIS-I observations and one {\em XMM-Newton} observation of X-ray emission from the ISM and the inner radio lobes of the nearby radio galaxy Centaurus A. The ISM has an average radial surface…

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

We studied the radio source associated with the ultraluminous X-ray source in NGC 5408 (L_X ~ 10^{40} erg/s). The radio spectrum is steep (index ~ -1), consistent with optically-thin synchrotron emission, not with flat-spectrum core…

天体物理学 · 物理学 2009-11-11 Roberto Soria , Rob Fender , Diana Hannikainen , Andrew Read , Ian Stevens

We present an XMM-Newton observation of the radio galaxy 4C 23.56 at z=2.48 which reveals extended X-ray emission coincident with the radio lobes spanning \~0.5 Mpc. These are the largest X-ray-bright lobes known at z>2. Under the…

天体物理学 · 物理学 2008-11-26 O. Johnson , O. Almaini , P. N. Best , J. Dunlop

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 radio and optical imaging and kinematic data for the radio galaxy Pictor A, including HST continuum and [OIII], emission-line images (at a resolution of 25 - 100 mas) and ground-based imaging and spectroscopy (at a resolution of…

天体物理学 · 物理学 2009-10-31 S. M. Simkin , E. M. Sadler , R. Sault , S. J. Tingay , J. Callcut

The radio components associated with the LMXB Sco X-1 have been monitored with extensive VLBI imaging at 1.7 and 5.0 GHz over four years, including a 56-hour continuous VLBI observation in 1999 June. We often detected one strong and one…

天体物理学 · 物理学 2009-11-06 E. B. Fomalont , B. J. Geldzahler , C. F. Bradshaw

We report Chandra imaging-spectroscopy and RXTE spectroscopy of the nearby, powerful radio galaxy Cygnus A. Various aspects of the results are discussed, including the X-ray properties of the nucleus, the radio hot spots, the cluster of…

天体物理学 · 物理学 2007-05-23 A. S. Wilson , K. A. Arnaud , D. A. Smith , Y. Terashima , A. J. Young

We study the emission of X-rays from lobes of FR-II radio galaxies by inverse Compton scattering of microwave background photons. Using a simple model that takes into account injection of relativistic electrons, their energy losses through…

宇宙学与河外天体物理 · 物理学 2015-05-19 Biman B. Nath

We have made ROSAT PSPC and HRI X-ray observations to study the intracluster gas surrounding the powerful radio source Hercules A. The cluster is luminous in X-rays (L_bol = 4.8x10^37 W), and the host of the radio source is the central…

天体物理学 · 物理学 2009-11-10 Nectaria A. B. Gizani , J. P. Leahy
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