Evolution of Disk-Embedded Objects

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Scientific paper

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Scientific paper

Giant planets, binary stars, and massive binary black hole systems are thought to be embedded in gaseous disks at some stage in their evolution. I will discuss some issues involving orbital and mass evolution of such embedded systems. The interactions are typically dominated by disk resonances which have been explored analytically. Multi-dimensional numerical simulations have also become a useful tool for exploring these interactions. Comparisons between analytical models and numerical simulations are important for testing the validity of models. I will describe some situations where resonances play a critical role and others where they play a lesser role.

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