Christian M. Fromm, Manel Perucho, Eduardo Ros, Petar Mimica, Tuomas Savolainen, Andrei P. Lobanov, J. Anton Zensus
The analysis of the radio light curves of the blazar CTA102 during its 2006
flare revealed a possible interaction between a standing shock wave and a
traveling one. In order to better understand this highly non-linear process, we
used a relativistic hydrodynamic code to simulate the high energy interaction
and its related emission. The calculated synchrotron emission from these
simulations showed an increase in turnover flux density, $S_{m}$, and turnover
frequency, $\nu_{m}$, during the interaction and decrease to its initial values
after the passage of the traveling shock wave.
View original:
http://arxiv.org/abs/1111.4844
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