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Convection-Dominated Accretion Flows with Radiative Cooling
作者姓名:李双良  薛力  卢炬甫
作者单位:Department of Physics and Institute of Theoretical Physics and Astrophysics, Xiamen University, Xiamen 361005
基金项目:Supported by the National Natural Science Foundation of China under Grant No 10673009.
摘    要:By numerically solving the set of basic equations describing black hole accretion flows with low accretion rates, we show that although the dynamical structure of these flows is essentially unaffected by radiative processes in comparison with the case in which the radiation is not considered, the radiative cooling can be more important than the advective cooling in the flow's convection-dominated zone, and this result may have implications to distinguish observationally convection-dominated accretion flows from advection-dominated accretion flows.

关 键 词:辐射制冷  流变学  对流  流体
收稿时间:2007-4-29
修稿时间:2007-04-29

Convection-Dominated Accretion Flows with Radiative Cooling
LI Shuang-Liang,XUE Li,LU Ju-Fu.Convection-Dominated Accretion Flows with Radiative Cooling[J].Chinese Physics Letters,2007,24(8):2451-2454.
Authors:LI Shuang-Liang  XUE Li  LU Ju-Fu
Institution:Department of Physics and Institute of Theoretical Physics and Astrophysics, Xiamen University, Xiamen 361005
Abstract:By numerically solving the set of basic equations describing black hole accretion flows with low accretion rates, we show that although the dynamical structure of these flows is essentially unaffected by radiative processes in comparison with the case in which the radiation is not considered, the radiative cooling can be more important than the advective cooling in the flow's convection-dominated zone, and this result may have implications to distinguish observationally convection-dominated accretion flows from advection-dominated accretion flows.
Keywords:97  60  Lf  98  62  Mw  95  30  Gv
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