Abstract
We report the discovery of unusually strong optical and X-ray emission associated with a knot in the radio jet of PKS B1421-490. The knot is the brightest feature observed beyond the radio band, with knot/core flux ratios 300 and 3.7 at optical and X-ray frequencies, respectively. We interpret the extreme optical output of the knot as synchrotron emission. The nature of the X-ray emission is unclear. We consider a second synchrotron component, inverse Compton emission from a relativistic, decelerating jet, and the possibility that this feature is a chance superposition of an unusual BL Lac object.
| Translated title of the contribution | The Knotty Question of the Jet of PKS B1421-490 |
|---|---|
| Original language | English |
| Pages (from-to) | L75 - L78 |
| Number of pages | 4 |
| Journal | Astrophysical Journal |
| Volume | 632 |
| Publication status | Published - 2005 |
Bibliographical note
Publisher: University of Chicago PressFingerprint
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