At radio and X-ray wavelengths, the nucleus is a strong source of synchrotron emission.
Observed linear polarization of the infrared radiation is consistent with synchrotron emission from the afterglow shock.
Relativistic jets emit most of their energy via synchrotron emission.
Beyond this radius synchrotron emission increases in the magnetized flow.
Jets and hotspots are the usual sources of high-frequency synchrotron emission.
Such synchrotron emission is expected from the environment around a supermassive black hole.
The radio emission is believed to be synchrotron emission from the jet.
As a result the radio plasma brightens in synchrotron emission.
He found that the light from the Crab Nebula was polarized, and produced by synchrotron emission.
This is needed when calculating the spectra for different types of synchrotron emission.
