Maximal Possible Accretion Rates for Slim Disks
By adopting the correct vertical gravitational force in studies of thermal equilibrium solutions, we find that there exists a maximal possible accretion rate for each radius in the outer region of optically thick accretion flows, such that only the inner regions of these flows can possibly take the form of slim disks.
Accretion and accretion disks Black hole Hydrodynamics
Wei-Min Gu Ju-Fu Lu
Department of Physics and Institute of Theoretical Physics and Astrophysics, Xiamen University, Xiamen, Fujian 361005, 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
405-407
2007-07-01(万方平台首次上网日期,不代表论文的发表时间)