A relativistic jet in the radio-quiet quasar PG 1407+263

Katherine M. Blundell*, Anthony J. Beasley, Geoffrey V. Bicknell

*Corresponding author for this work

    Research output: Contribution to journalArticlepeer-review

    52 Citations (Scopus)

    Abstract

    We present the results of a multiepoch radio monitoring campaign measuring the milliarcsecond structure of the jet in the radio-quiet quasar PG 1407+263. This is the highest sensitivity, highest resolution multiyear study of a distant active galaxy. The observations are naturally explained in terms of a beamed relativistic jet, some of whose fluctuations in flux density can be ascribed to interaction with the narrow-line region of the quasar. The optical properties of PG 1407+263, in particular the low equivalent widths of the emission lines, may be related to the fact that we are viewing this quasar almost pole-on, giving us a direct view into its broad-line region.

    Original languageEnglish
    Pages (from-to)L103-L106
    JournalAstrophysical Journal
    Volume591
    Issue number2 II
    DOIs
    Publication statusPublished - 10 Jul 2003

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