The knotty question of the jet of pks b1421-490
Sep, 20054 pages
Published in:
- Astrophys.J.Lett. 632 (2005) L75-L78
e-Print:
- astro-ph/0509205 [astro-ph]
DOI:
View in:
Citations per year
Abstract: (arXiv)
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.- galaxies: jets
- quasars: individual (PKS B1421-490)
References(25)
Figures(0)