Abstract
New multi-epoch Chandra observations, combined with multi-epoch, high-dynamic range VLA data, have allowed us to relate the radio and X-ray structure of the jet in Cen A to the jet dynamics. We present evidence that a significant fraction of the structure in the Cen A X-ray jet is due to particle acceleration at the interaction between the jet flow and internal galactic material.
Original language | English |
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Pages (from-to) | 116-121 |
Journal | Nuclear Physics B - Proceedings Supplements |
Volume | 132 |
Publication status | Published - Jun 2004 |
Keywords
- Astronomy