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Explore a 31-minute conference talk examining the crucial role of accretion in forming gravitational wave sources, presented by Pablo Marchant from KU Leuven. Delve into the complex interplay between circumbinary gas and binary systems, ranging from stellar pairs to supermassive black holes in galactic centers. Gain insights into the evolution of circumbinary gas, its influence on embedded binaries, and the most informative observational signatures. Learn about cutting-edge numerical techniques required to model these systems effectively. Understand how this presentation contributes to bridging the gap between massive black hole binary research and stellar binary studies, highlighting similarities across vastly different astrophysical scales. Discover the latest advancements in observations of stellar binaries and numerical modeling of both stars and black holes, setting the stage for future breakthroughs in the field.
