A binary star cosnsits of two stars A (mass $2.2 M_{s}$ ) and B (mass $11 M_{s}$ ) , where $M_{s}$ is the mass of the sun. they are separated by distance d and are rotating about their centre of mass, which is stationary. The ratio of the total angular momentum of the binary star to the angular momentum of star B about the centre of mass is

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A binary star cosnsits of two stars A (mass

2.2 M_{s}

) and B (mass

11 M_{s}

) , where

M_{s}

is the mass of the sun. they are separated by distance d and are rotating about their centre of mass, which is stationary. The ratio of the total angular momentum of the binary star to the angular momentum of star B about the centre of mass is

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A binary star cosnsits of two stars A (mass

2.2 M_{s}

) and B (mass

11 M_{s}

) , where

M_{s}

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