If two objects are in mutual revolution, then the period ($P$) with which they go around each other is related to the semi-major axis ($D$) of the orbit of one with the respect to the other
$D^3 = (M_1 + M_2)P^2$
$D$ is in astronomical units
$P$ is measured in years
$M_1 + M_2$ is the sum of the masses of the two stars in units of the Sun's mass