Other
Scientific paper
Jul 2007
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007dda....38.0401l&link_type=abstract
American Astronomical Society, DDA meeting #38, #4.01
Other
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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