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

doi:10.1016/s1387-6473(03)00095-2

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arXiv · astro-ph/0303327

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

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Abstract

We present results from a combined radio, optical, and X-ray study of the jet-associated emission features in NGC1052. 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.

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BibTeX RIS

M. Kadler, E. Ros, J. Kerp, H. Falcke, J. A. Zensus, R. W. Pogge, G. V. Bicknell. 2003-03-14. The Twin-Jet of NGC1052 at Radio, Optical, and X-ray Frequencies. https://doi.org/10.1016/s1387-6473(03)00095-2

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