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相关论文: Hydrodynamic Simulations of a Relativistic Jet Int…

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We present the results of three dimensional relativistic hydrodynamic simulations of interaction of AGN jets with a dense turbulent two-phase interstellar medium, which would be typical of high redshift galaxies. We describe the effect of…

高能天体物理现象 · 物理学 2016-06-15 Dipanjan Mukherjee , Geoffrey V. Bicknell , Ralph S. Sutherland , A. Y. Wagner

One of the most promising solutions for the cooling flow problem involves energy injection from the central AGN. However it is still not clear how collimated jets can heat the ICM at large scale, and very little is known concerning the…

天体物理学 · 物理学 2015-05-13 Elena Belsole , Andrew C. Fabian

We have performed the first three-dimensional relativistic hydrodynamic simulations of extragalactic jets of pure leptonic and baryonic plasma compositions propagating into a hydrostatic intracluster medium environment. The numerical…

高能天体物理现象 · 物理学 2017-06-28 Eunwoo Choi

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…

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…

高能天体物理现象 · 物理学 2015-06-05 Gayoung Chon , Hans Boehringer , Martin Krause , Joachim Truemper

Jets from active galactic nuclei (AGNs) are expected to heat the surrounding intracluster medium (ICM). We investigate how the interaction between jets and the ICM appears in high-resolution X-ray observations using mock X-ray observations…

星系天体物理 · 物理学 2026-01-14 Mahiro Shirotori , Yutaka Fujita

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

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…

高能天体物理现象 · 物理学 2015-06-05 William G. Mathews , Fulai Guo

The interaction between the radio plasma ejected by the active nucleus of a galaxy and the surrounding medium is a key process that can have a strong impact on the interstellar medium of the galaxy and hence on galaxy evolution. The closest…

星系天体物理 · 物理学 2015-11-10 F. Santoro , J. B. R. Oonk , R. Morganti , T. Oosterloo

We present the first stage of an investigation of the interactions of the jets in the radio galaxy Hydra A with the intracluster medium. We consider the jet kinetic power, the galaxy and cluster atmosphere, and the inner structure of the…

星系天体物理 · 物理学 2015-06-22 M. A. Nawaz , A. Y. Wagner , G. V. Bicknell , R. S. Sutherland , B. R. McNamara

We present the results of a deep search for associated radio features in the vicinity of the microquasar Cygnus X-3. The motivation behind is to find out evidence for interaction between its relativistic jets and the surrounding…

天体物理学 · 物理学 2009-11-11 J. Marti , D. Perez-Ramirez , J. L. Garrido , P. Luque-Escamilla , J. M. Paredes

We present an investigation of the X-ray absorption features predicted by hydrodynamic simulations of radio galaxies interacting with the intracluster medium (ICM) of their host galaxy clusters. We show how these absorption lines can be…

天体物理学 · 物理学 2009-11-11 Franziska Koeckert , Christopher S. Reynolds

Galactic jets are powerful energy sources reheating the intra-cluster medium in galaxy clusters. Their crucial role in the cosmic puzzle, motivated by observations, has been established by a great number of numerical simulations missing the…

宇宙学与河外天体物理 · 物理学 2015-05-28 Manel Perucho , Vicent Quilis , José María Martí

The interstellar medium of the radio galaxy IC 5063 is highly perturbed by an AGN jet expanding in the gaseous disc of the galaxy. We model this interaction with relativistic hydrodynamic simulations and multiphase initial conditions for…

A combination of three-dimensional (3D) magnetohydrodynamics (MHD) and synthetic numerical simulations are presented to follow the evolution of a randomly magnetised plasma that models the intra-cluster medium (ICM), under the isolated…

宇宙学与河外天体物理 · 物理学 2015-05-30 Martín Huarte-Espinosa , Martin Krause , Paul Alexander

We present numerical simulations investigating the interaction of AGN jets with galaxy clusters, for the first time taking into account the dynamic nature of the cluster gas and detailed cluster physics. The simulations successfully…

天体物理学 · 物理学 2009-11-11 S. Heinz , M. Brueggen , A. Young , E. Levesque

We present a multiwavelength study of the nucleus, environment, jets, and hotspots of the nearby FRII radio galaxy 3C 321, using new and archival data from MERLIN, the VLA, Spitzer, HST, and Chandra. An initially collimated radio jet…

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 3-D MHD and synthetic numerical simulations to follow the evolution of randomly magnetized intra-cluster medium plasma under the effects of powerful, light, hypersonic and bipolar jets. We prescribe the cluster magnetic field…

宇宙学与河外天体物理 · 物理学 2011-11-07 Martín Huarte-Espinosa , Martin Krause , Paul Alexander

We present three dimensional relativistic hydrodynamical simulations of a precessing jet interacting with the intracluster medium and compare the simulated jet structure with the observed structure of the Hydra A northern jet. For the…

星系天体物理 · 物理学 2016-02-24 M. A. Nawaz , G. V. Bicknell , A. Y. Wagner , R. S. Sutherland , B. R. McNamara
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