Monitoring of the superluminal quasar 4C 34.47

Details Monitoring of the superluminal quasar 4C 34.47 Monitoring of the superluminal quasar 4C 34.47

Jul 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992a%26a...261....1h&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 261, no. 1, p. 1-4.

Astronomy and Astrophysics

Astrophysics

16

Astronomical Interferometry, Quasars, Galactic Evolution, Galactic Nuclei, Galactic Structure, Very Long Base Interferometry

Scientific paper

10.7 GHz VLBI observations of the giant double-lobed quasar 4C 34.47 (1721 + 343) are presented. Previous VLBI monitoring at 5 GHz indicated the presence of superluminal motion in the core of this large radio source, at velocities of about 2.5/h c (Barthel et al., 1989). In the present observations, the superluminal nature of the apparent motions is confirmed. The evolution of the individual core components is studied in greater detail.

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