Published in
Kluwer, Symposium- International Astronomical Union, (121), p. 215-218, 1987
DOI: 10.1017/s0074180900155160
Observational Evidence of Activity in Galaxies, p. 215-218
DOI: 10.1007/978-94-009-3851-9_33
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Multifrequency Observations of the Seyfert Galaxy 3C 120 in 1983–1986
Journal article published in 1987 by
L. Maraschi,
W. Warnsteker,
L. Chiappetti 
,
S. Cristiani,
J. Danziger,
D. Danziger,
R. Falomo,
M. A. Malkan,
G. Tagliaferri,
E. G. Tanzi,
A. Treves,
W. Wamsteker
,
S. Cristiani,
J. Danziger,
D. Danziger,
R. Falomo,
M. A. Malkan,
G. Tagliaferri,
E. G. Tanzi,
A. Treves,
W. Wamsteker
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Abstract
3C 120 (z=0.033) has the optical spectrum typical of a Seyfert I Galaxy, however unlike most Seyfert Galaxies it exhibits strong radio emission with a compact component where VLBI observations indicated superluminal expansion. It could therefore be classified as a mini Radio Loud Quasar.