Add to ORKGWe model the spectral evolution of the synchrotron emission from the lobes of powerful FR II radio galaxies by combining an acceleration and transport model with a self-similar description of the hydrodynamics. Full details are given in Manolakou and Kirk [A&A 391 (2002) 127]
We present the first three-dimensional MHD radio galaxy simulations that explicitly model transport ...
Radio galaxies are among the largest and most powerful single objects known and are found at variety...
We present two-dimensional MHD simulations of the evolution of a young Type Ia supernova remnant dur...
We model the spectral evolution of the synchrotron emission from the lobes of powerful FR II radio g...
The spectral evolution of powerful double radio galaxies (FR II's) is thought to be determined by th...
We introduce a simple and economical but effective method for including relativistic electron transp...
This is the second in a series of papers presenting an analytical model for the evolu-tion of FRII r...
The recent discovery of the γ-ray emission from the lobes of the closest radio galaxy Centaurus A by...
Context. Radio-loud active galactic nuclei (AGNs) are thought to possess various sites of particle a...
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society....
The active galactic nuclei (AGN) lobe radio luminosities modelled in hydrodynamical simulations and ...
We have developed an economical, effective numerical scheme for cosmic-ray transport suitable for tr...
International audienceWe study the hotspots of powerful radiogalaxies, where electrons accelerated a...
We report on an effort to study the connections between dynamics in simulated radio galaxy plasma fl...
We have applied an effective numerical scheme for cosmic-ray transport to 3D MHD simulations of jet ...
We present the first three-dimensional MHD radio galaxy simulations that explicitly model transport ...
Radio galaxies are among the largest and most powerful single objects known and are found at variety...
We present two-dimensional MHD simulations of the evolution of a young Type Ia supernova remnant dur...
We model the spectral evolution of the synchrotron emission from the lobes of powerful FR II radio g...
The spectral evolution of powerful double radio galaxies (FR II's) is thought to be determined by th...
We introduce a simple and economical but effective method for including relativistic electron transp...
This is the second in a series of papers presenting an analytical model for the evolu-tion of FRII r...
The recent discovery of the γ-ray emission from the lobes of the closest radio galaxy Centaurus A by...
Context. Radio-loud active galactic nuclei (AGNs) are thought to possess various sites of particle a...
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society....
The active galactic nuclei (AGN) lobe radio luminosities modelled in hydrodynamical simulations and ...
We have developed an economical, effective numerical scheme for cosmic-ray transport suitable for tr...
International audienceWe study the hotspots of powerful radiogalaxies, where electrons accelerated a...
We report on an effort to study the connections between dynamics in simulated radio galaxy plasma fl...
We have applied an effective numerical scheme for cosmic-ray transport to 3D MHD simulations of jet ...
We present the first three-dimensional MHD radio galaxy simulations that explicitly model transport ...
Radio galaxies are among the largest and most powerful single objects known and are found at variety...
We present two-dimensional MHD simulations of the evolution of a young Type Ia supernova remnant dur...