Probing the Internal Structure of Magnetized, Relativistic Jets with Numerical Simulations

Probing the Internal Structure of Magnetized, Relativistic Jets with Numerical Simulations

From an observational point of view, unveiling the physical processes behind the nature of the jets emanating from radio-loud AGN demands the resolution of the structure across the jet with the highest angular resolutions. Relying on a magneto-fluid dynamical description, numerical simulations can h...

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Bibliographic Details
Main Author: José-María Martí
Format: Article
Language:English
Published: MDPI AG 2016-10-01
Series:Galaxies
Subjects:
galaxies: active
galaxies: jets
methods: numerical
MHD
shock waves
Online Access:http://www.mdpi.com/2075-4434/4/4/51

Internet

http://www.mdpi.com/2075-4434/4/4/51

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