Three-epoch VLBI observations of the nucleus in the lobe-dominated quasar 3C 334

Details Three-epoch VLBI observations of the nucleus in the lobe-dominated quasar 3C 334 Three-epoch VLBI observations of the nucleus in the lobe-dominated quasar 3C 334

Jul 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992apj...393...81h&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 393, no. 1, July 1, 1992, p. 81-86. Research supported by NASA and Trinity

Astronomy and Astrophysics

Astronomy

16

Astronomical Models, Maximum Entropy Method, Quasars, Radio Galaxies, Very Long Base Interferometry, Active Galactic Nuclei, Radio Jets (Astronomy), Radio Sources (Astronomy)

Scientific paper

VLBI observations at three epochs spanning 7 yr. reveals possible superluminal motion of the nucleus of the lobe-dominated quasar 3C 334. This is the third lobe-dominated quasar confirmed or suspected to be superluminal in a complete, flux density-limited sample of these objects, and the sixth including other surveys. The result continues the trend for lobe-dominated quasars to have lower superluminal speeds than core-dominated quasars, and coupled with other radio properties that are indicators of source orientation, it is consistent with the simple relativistic beaming model in a randomly oriented sample.

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