Abstract
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.
Sign-in/Register to access full text options 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
