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Issue A&A
Volume 425, Number 2, October II 2004
Page(s) 405 - 416
Section Extragalactic astronomy
DOI http://dx.doi.org/10.1051/0004-6361:20040546



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. Schlickeiser1

1  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

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© ESO 2004


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