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The Twin-Jet of NGC1052 at Radio, Optical, and X-ray Frequencies,
M. Kadler, E. Ros, J. Kerp, H. Falcke, J.A. Zensus, R.W. Pogge, G.V. Bicknell;br>
The Physics of Relativistic Jets in the CHANDRA and XMM Era,
G. Brunetti, D.E. Harris, R.M. Sambruna, & G. Setti (eds.), New Astronomy Reviews, in press (2003)
- Abstract
We present results from a combined radio, optical, and X-ray study of the
jet-associated emission features in NGC 1052. We analyse the
radio-optical morphology and find a good positional correlation between
the radio jet and the optical emission cone. Two optical emission knots
are directly associated with radio counterparts exhibiting a radio
to X-ray broadband spectrum not compatible with synchrotron emission.
We discuss the possibility that the thermal soft
spectrum of the extended X-ray emission originates from
jet driven shocks produced in the interaction between the jet-plasma and its
surrounding medium.
Eduardo Ros
ros@mpifr-bonn.mpg.de