Very light magnetized jets on large scales – I. Evolution and magnetic fields

Magnetic fields, which are undoubtedly present in extragalactic jets and responsible for the observed synchrotron radiation, can affect the morphology and dynamics of the jets and their interaction with the ambient cluster medium. We examine the jet propagation, morphology and magnetic field structu...

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Veröffentlicht in:	Monthly notices of the Royal Astronomical Society Jg. 400; H. 4; S. 1785 - 1802
Hauptverfasser:	Gaibler, V., Krause, M., Camenzind, M.
Format:	Journal Article
Sprache:	Englisch
Veröffentlicht:	Oxford, UK Blackwell Publishing Ltd 21.12.2009 Wiley-Blackwell Oxford University Press
Schlagworte:	Astronomy Earth, ocean, space Exact sciences and technology Fluid mechanics galaxies: clusters: general galaxies: jets Magnetic fields methods: numerical MHD Radio astronomy radio continuum: galaxies Stars & galaxies MHD galaxies: clusters: general magnetic fields galaxies: jets methods: numerical radio continuum: galaxies Plasma Magnetohydrodynamics Eccentricity Galaxies Kelvin Helmholtz instability Thermalization Numerical method Aspect ratio Helical field Continuum Dynamics Cosmic radio sources Magnetic structure Flux conservation Synchrotron radiation Mach number Discontinuity Turbulence Extragalactic jet Radio galaxies Astrophysical jets Galaxy clusters Morphology Models Magnetic fields
ISSN:	0035-8711, 1365-2966
Online-Zugang:	Volltext
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