Abstract
We have found evidence for interaction between a standing and a traveling shock in the jet of the blazar CTA 102. Our result is based in the study of the spectral evolution of the turnover frequency-turnover flux density (νm, Sm ) plane. The radio/mm light curves were taken during a major radio outburst in April 2006. © International Astronomical Union 2011.
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Fromm, C. M., Perucho, M., Savolainen, T., Ros, E., Lobanov, A. P., Zensus, J. A., & Lähteenmäki, A. (2010). Evidence for shock-shock interaction in the jet of CTA102. In Proceedings of the International Astronomical Union (Vol. 6, pp. 194–195). https://doi.org/10.1017/S1743921310016017
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