Correct Answer - B
`F_(min)=` gravitational foce between two outer stars `=(Gm^(2))/(4r)`
`F_(mM)=` gravitational force between central stars and outer star `=(GmM)/(r^(2))`
For circular motion outer star, `(mv^(2))/(r)=F_(min)+F_(mM)thereforev^(2)=(G(m+4M))/(4r)`
`T=` period of orbital motion `=(2pir)/(v)thereforem=(16pi^(2)r^(3))/(GT^(2))-4M=((150)/(16)-8)10^(30)=(11)/(8)xx10^(30)kg`