Key points are not available for this paper at this time.
In this paper the theory of spatial correlations developed in an earlier paper is applied to the discus- sion of the stability of binary stars, and a formula for estimating the time of dissolution, i-, of a binary is derived. It is found that (Mi + M2)'P T 4~'/2MNa3/2
S. Chandrasekhar (Sat,) studied this question.