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Related papers: Multiwavelength study of Cygnus A III. Evidence fo…

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The duty-cycle of powerful radio galaxies and quasars such as the prototype Cygnus A is poorly understood. X-ray observations of inverse-Compton scattered Cosmic Microwave Background (ICCMB) photons probe lower Lorentz-factor particles than…

Astrophysics · Physics 2009-11-13 K. C. Steenbrugge , K. M. Blundell , P. Duffy

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…

Astrophysics · Physics 2009-06-23 K. C. Steenbrugge , K. M. Blundell , P. Duffy

We present a spectral analysis of the lobes and X-ray jets of Cygnus A, using more than 2 Ms of $\textit{Chandra}$ observations. The X-ray jets are misaligned with the radio jets and significantly wider. We detect non-thermal emission…

High Energy Astrophysical Phenomena · Physics 2018-06-13 M. N. de Vries , M. W. Wise , D. Huppenkothen , P. E. J. Nulsen , B. Snios , M. J. Hardcastle , M. Birkinshaw , D. M. Worrall , R. T. Duffy , B. R. McNamara

Using deep Chandra ACIS observation data for Cygnus A, we report evidence of non-thermal X-ray emission from radio lobes surrounded by a rich intra-cluster medium (ICM). The diffuse X-ray emission, which are associated with the eastern and…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-18 Y. Yaji , M. S. Tashiro , N. Isobe , M. Kino , K. Asada , H. Nagai , S. Koyama , M. Kusunose

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…

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

We use 2.0 Msec of Chandra observations to investigate the cocoon shocks of Cygnus A and some implications for its lobes and jet. Measured shock Mach numbers vary in the range 1.18-1.66 around the cocoon. We estimate a total outburst energy…

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…

High Energy Astrophysical Phenomena · Physics 2015-06-23 Paul E. J. Nulsen , Andrew J. Young , Ralph P. Kraft , Brian R. McNamara , Michael W. Wise

The powerful FR II radio galaxy Cygnus A exhibits primary and secondary hotspots in each lobe. A 2 Msec Chandra X-ray image of Cygnus A has revealed an approximately circular hole, with a radius of 3.9 kpc, centered on the primary hotspot…

We present for the first time Very-Long-Baseline Interferometry images of the radio galaxy Cygnus A at the frequency of $86$ $\rm GHz$. Thanks to the high spatial resolution of only ${\sim}200$ Schwarzschild radii ($R_{\bf S}$), such…

High Energy Astrophysical Phenomena · Physics 2016-03-30 B. Boccardi , T. P. Krichbaum , U. Bach , M. Bremer , J. A. Zensus

Context. Cygnus A, as the nearest powerful FR II radio galaxy, plays an important role in understanding jets and their impact on the surrounding intracluster medium. Aims. To explain why the nucleus is observed superposed onto the eastern…

Astrophysics of Galaxies · Physics 2015-06-18 K. C. Steenbrugge , K. M. Blundell , S. Pyrzas

We present the detection of a radio-emitting jet from the black-hole candidate and X-ray binary source Cygnus X-1. Evidence of a bright core with a slightly extended structure was found on milliarcsecond resolution observations with the…

Cygnus A harbours the nearest powerful radio jet of an Fanaroff-Riley (FR) class II radio galaxy in a galaxy cluster where the interaction of the jet with the intracluster medium (ICM) can be studied in detail. We use a large set of Chandra…

High Energy Astrophysical Phenomena · Physics 2015-06-05 Gayoung Chon , Hans Boehringer , Martin Krause , Joachim Truemper

We present a detailed analysis of jet activity in the radio galaxy 3C348 at the center of the galaxy cluster Hercules A. We use archival Chandra data to investigate the jet-driven shock front, the radio-faint X-ray cavities, the eastern…

High Energy Astrophysical Phenomena · Physics 2025-01-15 F. Ubertosi , Y. Gong , P. Nulsen , J. P. Leahy , M. Gitti , B. R. McNamara , M. Gaspari , M. Singha , C. O'Dea , S. Baum

We describe approximate axisymmetric computations of the dynamical evolution of material inside radio lobes and X-ray cluster gas cavities in Fanaroff-Riley II sources such as Cygnus A. All energy is delivered by a jet to the lobe/cavity…

High Energy Astrophysical Phenomena · Physics 2015-06-05 William G. Mathews , Fulai Guo

At a distance of 249 Mpc ($z$=0.056), Cygnus A is the only powerful FR II radio galaxy for which a detailed sub-parsec scale imaging of the base of both jet and counter-jet can be obtained. Observing with VLBI at millimeter wavelengths is…

High Energy Astrophysical Phenomena · Physics 2015-04-07 Bia Boccardi , Thomas Krichbaum , Uwe Bach , Eduardo Ros , J. Anton Zensus

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…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-18 M. J. Hardcastle , J. H. Croston

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…

Astrophysics · Physics 2009-11-07 Curtis J. Saxton , Geoffrey V. Bicknell , Ralph S. Sutherland

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…

Astrophysics · Physics 2009-11-13 K. C. Steenbrugge , K. M. Blundell

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
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