Speaker
Ai-Jun Dong
() School of Physics and Electronic Science, Guizhou Normal University/Guizhou Provincial Key Laboratory of Radio Astronomy and Data Processing)
Description
It is very controversial whether the X-ray emission of strong radio black hole sources is from jet or acrretion disk. In this work, we collected a sample of radio loud and lower luminosity black hole sources (e.g., active galaxy nuclei and X-ray binaries) to explore their radio--X-ray correlation and fundamental plane of black hole actities. We consider the beaming effect on the radio emission and find that the X-ray--radio relation follow a shallower ($F_{\rm R}\propto F_{\rm X}^{\rm b}, b\sim 0.60$) and the fundamental plane is consisted with the result of Merloni et al.(2003). This results implied that the X-ray emission of strong radio black hole sources is originated from radiatively inefficient accretion mode (e.g., ADAF).
Primary authors
Ai-Jun Dong
() School of Physics and Electronic Science, Guizhou Normal University/Guizhou Provincial Key Laboratory of Radio Astronomy and Data Processing)
Bo-Wen Du
(Guizhou Provincial Key Laboratory of Radio Astronomy and Data Processing, Guizhou Normal University)
Wei-Long He
(School of Physics and Electronic Science, Guizhou Normal University/Guizhou Provincial Key Laboratory of Radio Astronomy and Data Processing)
Xue-Kun Zhang
(School of Physics and Electronic Science, Guizhou Normal University/Guizhou Provincial Key Laboratory of Radio Astronomy and Data Processing)
