Demircan, Osman2025-01-272025-01-2720051313-09272367-9522https://hdl.handle.net/20.500.12428/29128The orbital angular momentum distribution of interacting binary star systems and the important role of mass loss and the Alfven radius in effective spin down and orbital shrinkage (and thus in the orbital angular momentum evolution) of these systems are reviewed.eninfo:eu-repo/semantics/closedAccessArticle20248251N/AWOS:000433728700041