Strong structural variability in the lobe-dominated radio galaxy 3 C 111

Details Strong structural variability in the lobe-dominated radio galaxy 3 C 111 Strong structural variability in the lobe-dominated radio galaxy 3 C 111

Apr 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987a%26a...176..171g&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 176, no. 1, April 1987, p. 171-174.

Astronomy and Astrophysics

Astrophysics

14

Extragalactic Radio Sources, Galactic Structure, Radio Galaxies, Centimeter Waves, Flux Density, Galactic Nuclei

Scientific paper

High-resolution observations of the central component in 3 C 111 at 6 cm wavelength at two epochs show drastic changes in the structure of the compact emission region. The jet-like feature with two knots and a flux density of 600 mJy which was visible in 1980.4 had disappeared in 1985.4. This implies "superluminal behaviour" with a characteristic speed of >3 c.

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