Abstract
Evolution of a binary system with masses of 5m⊙ and 4m⊙, respectively, and with orbital period of 1.41 days is studied by means of non-stationary model calculations under assumptions of conservation of total mass and total orbital angular momentum of the system. As a result of mass exchange between the components we obtain a binary with masses of 8.46 and 0.54m⊙. Physical parameters of the final product indicate possible connection with shell stars.
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