The Knotty Question of the Jet of PKS B1421-490
arXiv:astro-ph/0509205 · doi:10.1086/497823
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. 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.
arXiv comment4 pages, 3 figures. Accepted to Astrophysical Journal Letters. Related materials and a higher resolution version of figure 1 may be obtained from our quasar jet survey page at http://space.mit.edu/home/jonathan/jets/
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Cited by in corpus (9)
- Large Scale Extragalactic Jets in the Chandra era I: data reduction and analysis
- An X-ray Imaging Survey of Quasar Jets -- Testing the Inverse Compton Model
- A Multi-Wavelength Study of the High Surface Brightness Hotspot in PKS1421-490
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