The last decade has been a golden epoch for the observations of extra- galactic jets. The extension of the observational window from the radio through infrared and optical up to the high energy band has provided us with a wealth of new data. The study of the jets by modeling their spectral energy distribution has become a very effective approach. Multi- band observations are determinant to constrain the model parameters and probe the radiative environment where the jets form and expand. The broadband fitting allows us to infer the main physical parameters of the emitting plasma and to consequently estimate the total jet kinetic power...
|Autori interni:||Migliori, Giulia|
|Titolo:||High Energy Emission in Relativistic Jets of AGN: Theory predictions and gamma-ray view|
|Data di pubblicazione:||ott-2010|
|Appare nelle tipologie:||8.1 PhD thesis|