The Dynamics of Radio Galaxies and Double-Double Radio Galaxies

Details The Dynamics of Radio Galaxies and Double-Double Radio Galaxies The Dynamics of Radio Galaxies and Double-Double Radio Galaxies

Dec 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011japa...32..477k&link_type=abstract

Journal of Astrophysics and Astronomy, Vol. 32, p. 477-486

Astronomy and Astrophysics

Astrophysics

Galaxies, Active, Galaxies, Jets, Galaxies, Nuclei, Radio Continuum, Galaxies, Galaxies, Individual, 3C457, J0041+3224

Scientific paper

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.

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