A visual binary is composed of two stars A and B. This visual binary has a rotation periodof 59.94 years and a distance of 3.64 pc from Earth. Assuming that the plane of the orbitis in the plane of the sky, the true angular extent of the semi-major axis is 7.61". The ratioof the distances of A and B from the centre of mass is aд/aB = 0.6. Find the masses ofeach member of the system.NOTE: to keep the calculation easier you should express the mass of the system in unitsof solar masses.

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