Astronomy and Astrophysics – Astrophysics – High Energy Astrophysical Phenomena
Scientific paper
2011-07-04
Astronomy and Astrophysics
Astrophysics
High Energy Astrophysical Phenomena
Poster on the International Meeting "Understanding Relativistic Jets", Krakow, May 23-26, 2011
Scientific paper
The observed shift of the core of the relativistic AGN jets as a function of frequency allows us to evaluate the number density of outflowing plasma and, hence, the magnetization parameter. New analysis of more than 20 sources shows that for most of jets the magnetization parameter ~ 10 - 100. Since the magnetization parameter is the maximum possible bulk Lorentz-factor of the relativistic flow, this estimate is consistent with the observed superluminal motion.
Beskin Vasilii S.
Kovalev Yu. Yu.
Nokhrina Elena E.
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