EVOLUTION OF NON-THERMAL EMISSION FROM SHELL ASSOCIATED WITH AGN JETS
作者： Hirotaka Ito , Motoki Kino , Nozomu Kawakatu , Shoichi Yamada
DOI: 10.1088/0004-637X/730/2/120
关键词: Synchrotron radiation 、 Quasar 、 Radiative cooling 、 Photon 、 Astrophysics 、 Physics 、 Radiation 、 Scattering 、 Active galactic nucleus 、 Emission spectrum
摘要: We explore the evolution of emissions by accelerated electrons in shocked shells driven jets active galactic nuclei (AGNs). Focusing on powerful sources which host luminous quasars, we evaluated broadband emission spectra properly taking into account adiabatic and radiative cooling effects electron distribution. The synchrotron radiation inverse Compton (IC) scattering various photons that are mainly produced accretion disc dusty torus considered as processes. show resultant is dominated IC for compact (. 10kpc), whereas more important larger sources. also compare shell with those expected from lobe under assumption a fractions energy deposited carried non-thermal
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