Palestrante
Descrição
Observations of high-energy emissions in relativistic astrophysical jets show the existence of particle acceleration, the study of these emissions can help us understand the acceleration mechanisms that these particles may be suffering. It is believed that in these jets within active galactic nuclei the particles get accelerated to extreme speeds via Fermi-type acceleration, mainly along the magnetic field lines. With the Cherenkov Telescope Array Observatory (CTAO), which will have five-to twenty-times better sensitivity than the current generation of Imaging Atmospheric Cherenkov Telescopes depending on energy, we will be able to better understand the nature of the acceleration processes in these astrophysical objects. In this poster, we will show the preliminary results of the modeling of high-energy leptonic emissions of astrophysical jets sources (3C-264, IC 310 and PKS 0625-35) especially their spectral energy distribution (SED), and their detectability by CTAO.
