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Jet speed, beaming & sidedness, and all that

Kundt, Wolfgang

Hot Spots in Extragalactic Radio Sources, 2005, p.179-184

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Título:
Jet speed, beaming & sidedness, and all that
Autor: Kundt, Wolfgang
Assuntos: Bulk Lorentz Factor ; Extragalactic Radio Source ; Lorentz Factor ; Radio Galaxy ; Total Spectral Power
É parte de: Hot Spots in Extragalactic Radio Sources, 2005, p.179-184
Descrição: It is argued that the astrophysical jets consist of quasi-monoenergetic relativistic pair plasma, of Lorentz factor ℓ = 105±3, performing a quasi-lossfree \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document} vec E \times \vec B \end{document}-drift in equi-pressure convected fields. The Lorentz factor derived from the naive beaming formula (in unified schemes) has no physical meaning. Hydrodynamical and hydromagnetic jet simulations agree with reality in as much as that they satisfy the conservation laws. Multiple hotspots may result from beam swinging.
Títulos relacionados: Lecture Notes in Physics
Editor: Berlin, Heidelberg: Springer Berlin Heidelberg
Idioma: Inglês

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