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A New Geometry for Superluminal Motions

Published online by Cambridge University Press:  04 August 2017

Marco Salvati
Marco Salvati*
Affiliation:
European Southern Observatory, Garching, FRG *)

Abstract

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In the context of superluminal motions, the statistical difficulties intrinsic to the canonical jet geometry are alleviated if the relativistic flows occur on a plane screen, orthogonal to the source axis. The strongest superluminal effects should be detected when the source lies in the plane of the sky, rather than pointing at the observer. The polarization properties, the simplest deviations from the basic geometry, and the connection with other non-thermal phenomena are also indicated.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 110: VLBI and Compact Radio Sources , 1984 , pp. 239 - 242
Copyright
Copyright © Reidel 1984 

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