3C 380 contains a complex radio structure. Radio images produced by the
very long baseline interferometry (VLBI) at 5
GHz, showed the source is mainly extended, containing several components including a compact radio core and a ridge of extended
radio emission. In additional, the quasar also has a diffused halo with a
spectral index of 1.0 ± 0.2 which represents a common feature of the radio lobes in
Fanaroff-Riley class II quasars. There are also two hotpots located in northwest direction. The
radio jet of 3C 380 on parsec-scales is known to be bent. Based on VLBI observations, it is shown to be resolved when travelling in a
transverse direction, however it also shows signs of rapid
brightness variations unlike other nuclear jets indicating phase effects play a role in causing these changes. Apart from that, the jet shows
superluminal motion and a
Faraday rotation gradient measuring 70-200
parsecs in width across it. Radio imaging
Very Long Baseline Array (VLBA) also finds the jet is extending in a northwest direction. According to
Hubble Space Telescope (HST) and VLBA, the jet has two knots. These knots are respectively named as knot 1, located 0.73
arcseconds from the core and knot 2 which is located 0.4 arcseconds away from the former. Together, these knots are found laid over lobelike emission which in turn, is stretched out in both east and northeast directions. Multifrequency
polarization have also been found in 3C 380. Based on observations, both the core and jet contains polarization by 6
percent, while the other component has 16 percent polarization. Enhanced
flux density at 24 GHz from the object was also detected in September 2020. == References ==