The Dynamics of Radio Galaxies and Double-Double Radio Galaxies
Saikia, D. J.
Relativistic and magnetized plasma ejected by radio loud AGNs through jets form the diffuse lobes of radio galaxies. The radiating particles (electron/electron-positron) in lobes emit in radio via the synchrotron process and X-ray via inverse-Compton scattering of cosmic microwave background photons. The thermal environment around radio galaxies emits X-rays via the thermal bremsstrahlung process. By combining information from these processes we can measure physical conditions in and around the radio lobes and thus study the dynamics of radio galaxies, including double-double radio galaxies.
Published inJournal of Astrophysics and Astronomy
RelationsSchool of Physics, Astronomy and Mathematics
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