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Relativistic Numerical Simulations of Superluminal Sources

Published online by Cambridge University Press:  12 April 2016

J.L. Gómez ,
J. Mª. Martí ,
A.P. Marscher ,
J. Mª. Ibáñez  and
A. Alberdi
J.L. Gómez
Affiliation:
Instituto de Astrofísica de Andalucía (CSIC), Granada, Spain
J. Mª. Martí
Affiliation:
Departamento de Astronomía y Astrofísica, Universidad de Valencia, Valencia, Spain
A.P. Marscher
Affiliation:
Department of Astronomy, Boston University, Boston, USA
J. Mª. Ibáñez
Affiliation:
Departamento de Astronomía y Astrofísica, Universidad de Valencia, Valencia, Spain
A. Alberdi
Affiliation:
Instituto de Astrofísica de Andalucía (CSIC), Granada, Spain

Abstract

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We study the generation and evolution of superluminal components in relativistic jets through relativistic hydrodynamical and emission simulations of a square-wave perturbation in the jet velocity.

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 164: Radio Emission from Galactic and Extragalactic Compact Sources , 1998 , pp. 49 - 50
Copyright
Copyright © Astronomical Society of the Pacific 1998

References

Gómez, J.L., et al. 1997. ApJ, 482, L33–36.Google Scholar
Marscher, A.P., et al. 1997. BAAS, 29, 847.Google Scholar
Martí, J.|Mª. et al. 1997. ApJ, 479, 151–163.CrossRefGoogle Scholar