A possible superluminal motion of the VLBI core in the quasar 3C345

Details A possible superluminal motion of the VLBI core in the quasar 3C345 A possible superluminal motion of the VLBI core in the quasar 3C345

Dec 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992acasn..33..352q&link_type=abstract

Acta Astronomica Sinica (ISSN 0001-5245), vol. 33, no. 4, p. 352-361.

Astronomy and Astrophysics

Astronomy

Quasars, Stellar Cores, Stellar Oscillations, Space Observations (From Earth), Stellar Models, Very Long Base Interferometry

Scientific paper

A precise method is used to derive the apparent motion of the core in
the south-north direction and the common path of the intrinsic motion of
the knots in the quasar 3C345. The apparent motion derived for the core
is found to be oscillatory and the maximum apparent speed is about
0.10-0.15 mas/yr.

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