Parsec-scale shocks in the kiloparsec-scale jet of Centaurus A

Abstract

High angular resolution VLBI observations of Centaurus A have been undertaken that allow access to a wide field-of-view, encompassing both the well-studied pc-scale jet and the inner part of the kpc-scale jet. The VLBI observations have detected compact regions of synchrotron emission in the kpc-scale jet that coincide with three stationary features identified from previous VLA monitoring observations. Each of these stationary features is associated with strong localised X-ray emission. The VLBI results strengthen arguments made by previous authors suggesting that the stationary features may be the result of stellar objects or gas clouds traversing the jet flow, intercepting the jet and causing strong shocks. The VLBI data show that the most strongly shocked regions in these features are resolved but have extents no larger than a few pc, reducing the required mass of the typical intercepting object by a factor of ~10 relative to previous estimates, making explanations based on high mass loss stars or low density gas clouds more plausible.

Submitted to the Astronomical Journal. 18 pages, 3 figures

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• The radio structure of 3C 316, a galaxy with double-peaked narrow optical emission lines
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• Cosmic Ray Ionization of Low-Excitation Lines in Active Galactic Nuclei and Starburst Galaxies
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• The Subparsec-scale Structure and Evolution of Centaurus A. III. A Multi-Epoch Spectral And Polarimetric VLBA Study
• The origin of the very-high-energy radiation along the jet of Centaurus A