Eject and disconnect the LeapStart device from your computer. The power light will flash green when content is downloading. Follow the instructions in the LeapFrog Connect Application to set up your LeapStart system and download companion audio and video for each of your books. For the clumpy structure to be maintained over long period, the incident radiation field needs to be sufficiently weaken for most of the clumps, or, some mechanism that creates the clumps continuously is needed. Started to install the LeapFrog Connect Application. A simple estimate suggests that the clumps are destroyed in time-scales shorter than their orbital periods. We discuss the influences of the AGN radiation on the clumpy torus. We perform three-dimensional radiation hydrodynamic simulations of uniform dusty gas clouds irradiated by an active galactic nucleus (AGN) to investigate the dependence of evolution of clouds on the ionization parameter $\mathcal $. Three-dimensional radiation hydrodynamic simulations On the evolution of gas clouds exposed to AGN radiation I. On the evolution of gas clouds exposed to AGN radiation I.
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