The knotty question of the jet of pks b1421-490

Sep, 2005
4 pages
Published in:
  • Astrophys.J.Lett. 632 (2005) L75-L78
e-Print:

Citations per year

200920132017202120232031
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)