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相关论文: The X-Ray Cavity Around Hotspot E in Cygnus A: Tun…

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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

We have mapped the powerful radio galaxy Hercules A at six frequencies spanning 1295 to 8440 MHz using the VLA in all four configurations. Here we discuss the structure revealed in total intensity, spectral index, polarization, and…

天体物理学 · 物理学 2009-11-07 Nectaria A. B. Gizani , J. P. Leahy

We present the discovery of a 4 kpc molecular gas lane in the Cygnus A host galaxy, using ALMA CO 2-1 observations. The gas lane is oriented roughly perpendicular to the projected radio jet axis. The CO emission generally follows the clumpy…

星系天体物理 · 物理学 2022-10-12 C. L. Carilli , R. A. Perley , D. A. Perley , V. Dhawan , R. Decarli , A. Evans , K. Nyland

We report two simulations that have been carried out at the SX-5 at HLRS (Stuttgart). One simulation is axisymmetric and purely hydrodynamic, but with a resolution of 20 points per beam-radius (ppb). The bipolar jet is injected in the…

天体物理学 · 物理学 2007-05-23 Martin G. H. Krause , Max Camenzind

A 227 ksec Chandra Observatory X-ray image of the hot plasma in the Hydra A cluster has revealed an extensive cavity system. The system was created by a continuous outflow or a series of bursts from the nucleus of the central galaxy over…

天体物理学 · 物理学 2011-02-11 M. W. Wise , B. R. McNamara , P. E. J. Nulsen , J. C. Houck , L. P. David

We present new Karl G. Jansky Very Large Array (VLA, 1.5 GHz) radio data for the giant elliptical galaxy IC 4296, supported by archival radio, X-ray (Chandra, XMM-Newton) and optical (SOAR, HST) observations. The galaxy hosts powerful radio…

We study the jet and counterjet of the powerful classical double FRII radio galaxy Cygnus A as seen in the 5, 8 and 15-GHz radio bands using the highest spatial resolution and signal-to-noise archival data available. We demonstrate that the…

天体物理学 · 物理学 2009-11-13 K. C. Steenbrugge , K. M. Blundell

Images made with the VLBA have resolved the region in a nearby radio galaxy, Pictor A, where the relativistic jet that originates at the nucleus terminates in an interaction with the intergalactic medium, a so-called radio galaxy hot spot.…

天体物理学 · 物理学 2009-11-13 S. J. Tingay , E. Lenc , G. Brunetti , M. Bondi

We present a 200 ks Chandra ACIS-I image of Cygnus A, and discuss a long linear feature seen in its counterlobe. This feature has a non-thermal spectrum and lies on the line connecting the brighter hotspot on the approaching side and the…

天体物理学 · 物理学 2009-06-23 K. C. Steenbrugge , K. M. Blundell , P. Duffy

We report detailed studies of the X-ray emission from the kpc scale jet in the nearest active galaxy, Cen A. 41 compact sources were found within the jet, 13 of which were newly identified. We construct the luminosity function for the…

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

Vast cavities in the intergalactic medium are excavated by radio galaxies. The cavities appear as such in X-ray images because the external medium has been swept up, leaving a hot but low density bubble surrounding the radio lobes. We…

星系天体物理 · 物理学 2021-01-12 Michael D. Smith andJustin Donohoe

We employ MUSE/VLT data to study the ionised and highly ionised gas phases of the feedback in Circinus, the closest Seyfert 2 galaxy to us. The analysis of the nebular emission allowed us to detect a remarkable high-ionisation gas outflow…

星系天体物理 · 物理学 2021-06-28 M. A. Fonseca-Faria , A. Rodríguez-Ardila , M. Contini , V. Reynaldi

PKS B2152-699 has radio power characteristic of sources that dominate radio feedback. We present new deep ATCA, Chandra and optical observations, and test the feedback model. We report the first high-resolution observations of the radio…

高能天体物理现象 · 物理学 2015-06-05 D. M. Worrall , M. Birkinshaw , A. J. Young , K. Momtahan , R. A. E. Fosbury , R. Morganti , C. N. Tadhunter , G. Verdoes Kleijn

Double-lobed radio galaxies a few 100s of kpc in extent, like Cygnus A, are common at redshifts of 1 to 2, arising from some 10 per cent of the most powerful Active Galactic Nuclei (AGN). At higher redshifts they are rare, with none larger…

高能天体物理现象 · 物理学 2015-06-19 A. C. Fabian , S. A. Walker , A. Celotti , G. Ghisellini , P. Mocz , K. M. Blundell , R. G. McMahon

We present millimetre photometry and submillimetre imaging of the central core and two hotspots in the radio lobes of the galaxy Cygnus-A. For both hotspots and the central core the synchrotron spectrum continues smoothly from the radio to…

天体物理学 · 物理学 2009-10-31 E. I. Robson , L. L. Leeuw , J. A. Stevens , W. S. Holland

We present subarcsecond resolution mid-infrared images at 10.8 and 18.2 microns of Cygnus A. These images were obtained with the University of Florida mid-IR camera/spectrometer OSCIR at the Keck II 10-m telescope. Our data show extended…

We report the first observation of a transient relativistic jet from the canonical black hole candidate, Cygnus X-1, obtained with the Multi-Element Radio-Linked Interferometer Network (MERLIN). The jet was observed in only one of six…

The compact radio source Sgr A* is coincident with a 4 million solar mass black hole at the dynamical center of the Galaxy and is surrounded by dense orbiting ionized and molecular gas. We present high resolution radio continuum images of…

高能天体物理现象 · 物理学 2015-06-11 F. Yusef-Zadeh , R. Arendt , H. Bushouse , W. Cotton , D. Haggard , M. W. Pound , D. A. Roberts , M. Royster , M. Wardle

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…