Search results for "relativistic processes ISM: jets and outflows"

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Dissipative Processes and Their Role in the Evolution of Radio Galaxies

2019

Particle acceleration in relativistic jets to very high energies occurs at the expense of the dissipation of magnetic or kinetic energy. Therefore, understanding the processes that can trigger this dissipation is key to the characterization of the energy budgets and particle acceleration mechanisms at action in active galaxies. Instabilities and entrainment are two obvious candidates to trigger dissipation. On the one hand, supersonic, relativistic flows threaded by helical fields, as expected from the standard formation models of jets in supermassive black-holes, are unstable to a series of magnetohydrodynamical instabilities, such as the Kelvin-Helmholtz, current-driven, or possibly the p…

Active galactic nucleuslcsh:AstronomyRadio galaxyAstrophysics::High Energy Astrophysical Phenomenagalaxies: activeFOS: Physical sciencesKinetic energy01 natural scienceslcsh:QB1-991X-rays: binariesAstrophysical jet0103 physical sciencesrelativistic processes ISM: jets and outflows010303 astronomy & astrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsJet (fluid)010308 nuclear & particles physicsAstronomy and AstrophysicsMechanicsgalaxies: jetsradiation mechanisms: non-thermalDissipationAstrophysics - Astrophysics of GalaxiesParticle accelerationAstrophysics of Galaxies (astro-ph.GA)MagnetohydrodynamicsAstrophysics - High Energy Astrophysical PhenomenamagnetohydrodynamicsGalaxies
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