Is 3C287 a precessing radio source?
Received 24 March 1998 / Accepted 22 June 1998
We present a 5 GHz VLBI image of the compact steep spectrum (CSS) quasar 3C287. The source has been one of the candidate precessing CSS sources. Both static features and large structural changes are observed since the earliest VLBI experiments. The overall picture does not seem to support a precessing jet scenario.
Key words: galaxies: active radio continuum: galaxies quasars: individual: 3C287
Send offprint requests to: Z. Paragi, 1st address
© European Southern Observatory (ESO) 1998
Online publication: September 17, 1998