Understanding our Galactic center and other Low-luminosity AGNs
This review summarizes our current understanding of low-luminosity AGNs in the context of the advection- dominated accretion flow (ADAF). Special attention is paid to the best investigated Source, the supermassive black hole in our galactic center, Sgr A. ADAF can naturally explain the most important features of these sources such as the low luminosity and the lack of the big blue bump in their spectral energy distribution. The emission from the jet usually dominates over the ADAF in the radio waveband and sometimes in other wavebands as well especially the X-ray.
Radiation mechanisms-Accretion and accretion disks-Galactic center-active galactic nuclei-jets
Feng Yuan
Shanghai Astronomical Observatory, Chinese Academy of Sciences, Nandan Road 80, Shanghai 200030, China
国际会议
紧凑型物体的天体物理学国际会议(International Conference on Astrophysics of Compact Objects)
安徽黄山
英文
361-368
2007-07-01（万方平台首次上网日期，不代表论文的发表时间）