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The Knotty Question of the Jet of PKS B1421-490

  • JM Gelbord
  • , HL Marshall
  • , DM Worrall
  • , M Birkinshaw
  • , JEJ Lovell
  • , R Ojha
  • , L Godfrey
  • , DA Schwartz
  • , ES Perlman
  • , M Georganopoulos
  • , DW Murphy
  • , DL Jauncey

Research output: Contribution to journalArticle (Academic Journal)peer-review

8 Citations (Scopus)

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 contributionThe Knotty Question of the Jet of PKS B1421-490
Original languageEnglish
Pages (from-to)L75 - L78
Number of pages4
JournalAstrophysical Journal
Volume632
Publication statusPublished - 2005

Bibliographical note

Publisher: University of Chicago Press

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