Numerical modelling of the lobes of radio galaxies in cluster environments – II. Magnetic field configuration and observability

We describe three-dimensional magnetohydrodynamical modelling of powerful radio galaxies in realistic poor cluster environments. This modelling extends our earlier work on the hydrodynamics of radio galaxies as a function of their cluster environment to consider the magnetic field configuration in t...

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Veröffentlicht in:	Monthly notices of the Royal Astronomical Society 2014-09, Vol.443 (2), p.1482-1499
Hauptverfasser:	Hardcastle, M. J., Krause, M. G. H.
Format:	Artikel
Sprache:	eng
Schlagworte:	Astronomy Cosmic rays Fluid mechanics Magnetic fields Stars & galaxies
Online-Zugang:	Volltext
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