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A&A 425, 405-416 (2004)
DOI: 10.1051/0004-6361:20040546
The impact of thermal gas in AGN jets on the low-frequency emission
M. Siewert1, M. Pohl1, 2 and R. Schlickeiser11 Institut für Theoretische Physik, Lehrstuhl IV, Ruhr-Universität Bochum, 44780 Bochum, Germany
e-mail: ms@tp4.ruhr-uni-bochum.de
2 Department of Physics and Astronomy, Iowa State University, Ames, IA 50011, USA
(Received 29 March 2004 / Accepted 25 May 2004)
Abstract
We study the effect of non-relativistic, thermal matter in the jets of
active galaxies (AGN)
on the low-frequency non-thermal emission and the variability thereof. In
matter-dominated jets, sizable quantities of gas should exist, in particular
in the compression zones near the collision fronts that are an implicit ingredient of
Fermi-type particle acceleration scenarios. Non-relativistic thermal gas in AGN jets
noticably contributes to the optical depth at radio to infrared frequencies, and much less
to the emission, with an efficiency that is strongly temperature-dependent.
The observable flux of
low-frequency emission is thus modulated by the temperature evolution of the
thermal gas, and it can therefore display very complicated variability.
For a particular particle energisation scenario we calculate the temperature evolution of the thermal
plasma as well as the radiation transport of low-frequency emission, and thus derive simulated
light curves at different frequencies and their typical correlation properties.
Key words: galaxies: active -- plasmas
SIMBAD Objects
© ESO 2004
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