Speaker
Hanrong WU Hanrong
(高能所)
Description
Based on current observations, the main conclusion derived from applying the single-zone conical jet synchrotron self-Compton model to the data is that this model requires a critically low magnetization, which is insonsistent with radio observations of nearby radio galaxies. Therefore, with the current dataset, we cannot favor or disfavor any of the considered models. Probing fast variability at very high energies (VHE) and variability across different frequencies, particularly between the X-ray and VHE bands, is likely the most powerful tool to test emission models. Consequently, observations by LHAASO are crucial and may provide important observational evidence.
Primary author
Hanrong WU Hanrong
(高能所)
