In a double star system, two stars of masses m_(1)and m_2 seperated by a distance d rotate about their centre of mass. Then their common angular velocity would be:

In a double star system, two stars of masses m_(1)and m_2 seperated by

1.	In a double star system, two stars of masses m_(1)and m_2 seperated by a distance d rotate about their centre of mass. Then their common angular velocity would be:
Answer» `sqrt((Gm_(1))/d^(3))` `sqrt((Gm_(2))/d^(3))` `sqrt((G(m_(1)+ m_(2)))/d^(3))` `sqrt(d^(3)/(G(m_(1) + m_(2))))` Answer :C