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Directivity Pattern Simulation of the Jet Radio Emission

Published online by Cambridge University Press:  19 July 2016

Y.Y. Kovalev
Y.Y. Kovalev*
Affiliation:
Astro Space Center, Lebedev Physical Institute Profsojuznaja street, 84/32 117810, Moscow Russia

Extract

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Recently the 1.5 years flux observations of a quasar 0235+16 at 8 frequencies have been explained by the emission of a jet in a strong radial magnetic field of an AGN (in according with the Hedgehog model, suggested by N.S. Kardashev in 1969; see poster by Kovalev Y.Y. and Larionov G.M. to this Symposium).

Type
Poster Contributions: Radio Emission (Maps)
Information
Symposium - International Astronomical Union , Volume 159: Multi-Wavelength Continuum Emission of AGN , 1994 , pp. 428
Copyright
Copyright © Kluwer 1994 

References

Blandford, R.D. and Koenigl, A. 1979. Asrophys. J. V. 232. P.34.Google Scholar