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The Radio Jet of Quasar 0153+744

Published online by Cambridge University Press:  12 April 2016

C.A. Hummel
C.A. Hummel*
Affiliation:
Universities Space Research Association, c/o US Naval Observatory - AD 5, Washington DC 20392, USA

Abstract

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We highlight a few aspects of the radio jet of quasar 0153+744. Some challenge the relativistic beaming model to explain a stationary jet of short length and ending in a bright secondary component, extreme bending of the jet, and the lack of any emission on the counter jet side. We discuss a model of a precessing mildly relativistic jet for 0153+744.

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 164: Radio Emission from Galactic and Extragalactic Compact Sources , 1998 , pp. 61 - 62
Copyright
Copyright © Astronomical Society of the Pacific 1998

References

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