no code implementations • 6 Dec 2020 • Xiaotong Guo, Qiusheng Gu, Nan Ding, Xiaoling Yu, Yongyun Chen
We also find that CT AGNs have a higher Eddington ratio than non-CT AGNs, and that both CT AGNs and non-CT AGNs show similar properties of host galaxies.
Astrophysics of Galaxies High Energy Astrophysical Phenomena
