no code implementations • 24 Dec 2020 • Xiao-Li Huang, Ze-Rui Wang, Ruo-Yu Liu, Xiang-Yu Wang, En-Wei Liang
In the wind medium with $A_{\ast}> 0. 1$, the cascade emission in the eV-GeV band is comparable or even larger than the emission of the primary electrons at early time.
High Energy Astrophysical Phenomena
no code implementations • 19 May 2020 • Can Tan, Rui Xue, Lei-Ming Du, Shao-Qiang Xi, Ze-Rui Wang, Zhao-Hua Xie
(4) There is an anti-correlation between the peak energy of SEDs ($\gamma_{\rm peak}$) and the jet power ($P_{\rm jet}$), which is consistent with the blazar sequence.
High Energy Astrophysical Phenomena
