High-resolution studies of the twin jet in NGC 1052
  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. 
E. Ros (MPIfR), M. Kadler (Bamberg Obs., ECAP, CRESST/NASA GSFC, &   USRA), Y.Y. Kovalev (MPIfR, ASC Lebedev), H.D. Aller (U...