Structural changes in the nucleus of the double radio galaxy 3C 390.3

Details Structural changes in the nucleus of the double radio galaxy 3C 390.3 Structural changes in the nucleus of the double radio galaxy 3C 390.3

Mar 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988a%26a...192...53a&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 192, no. 1-2, March 1988, p. 53-56.

Astronomy and Astrophysics

Astronomy

25

Active Galactic Nuclei, Galactic Structure, Radio Galaxies, Radio Jets (Astronomy), Very Long Base Interferometry

Scientific paper

The radio galaxy 3C 390.3 is one of a class of symmetric extended double radio sources with a relatively strong compact central component. VLBI observations made on four occasions since 1976 show features which suggest superluminal motion in the direction of the northwest extended lobe. If superluminal motion in 3C 390.3 is confirmed, interpretation in terms of relativistic jet models suggests that bulk relativistic motion must be common in the central components of extended extragalactic radio sources.

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