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arXiv · 0812.0280

High-resolution studies of the twin jet in NGC 1052

E. Ros·M. Kadler·Y. Y. Kovalev·H. D. Aller·M. F. Aller·S. Kaufmann
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Abstract

The radio loud galaxy NGC 1052 is being studied in an intensive multi-band campaign including X-ray brigthness monitoring and spectroscopic observations, single-dish radio brightness monitoring at centimetre wavelengths, and a high-frequency very-long-baseline interferometry monitoring program. Here we present a progress report on our studies from this program. The final goal of our observations is to relate the findings from the high-resolution radio images with the observed variations in the X-ray regime, to address the accretion processes and their relationship with the radio jet activity.

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E. Ros, M. Kadler, Y. Y. Kovalev, H. D. Aller, M. F. Aller, S. Kaufmann. 2008-12-01. High-resolution studies of the twin jet in NGC 1052. https://arxiv.org/abs/0812.0280

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