  We have studied the inner regions of the LINER galaxy NGC1052 since the mid
1990s at high resolution with 15 GHz very-long-baseline interferometry
observations. A compact, two-sided jet structure is revealed, with multiple
sub-parsec scale features moving outward from the central region with typical
speeds of 0.26 c. Complementary to this, since early 2005 we are performing a
multi-mission campaign of observations of this source, including X-ray
spectroscopy, X-ray, and radio flux density monitoring, and VLBA observations
at 22 GHz and 43 GHz. X-ray variability is present at time scales of weeks,
comparable with the structural changes observed by VLBI. Here we present first
results of the high-resolution imaging observations and discuss these findings
in the context of the multi-band campaign.
