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This course aims to explore the evolution and influence of circumbinary gas on binary systems, focusing on both stellar and black hole binaries. Participants will learn about observational signatures of circumbinary gas, novel numerical techniques for modeling these systems, and the similarities in problems across different astrophysical scales. The teaching method involves presentations and discussions led by experts in the field. This course is intended for researchers and professionals working in astrophysics, particularly those interested in binary systems and their accretion processes.
