Two stars of masses $M$ and $2M$ are at a distance $d$ apart and are revolving around their common center of mass. The angular velocity of the system of the two stars is ($G$ is the universal gravitational constant).

  • A
    $\sqrt{\frac{4 G M}{d^3}}$
  • B
    $\sqrt{\frac{2 G M}{d^3}}$
  • C
    $\sqrt{\frac{9 G M}{d^3}}$
  • D
    $\sqrt{\frac{3 G M}{d^3}}$

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