Stability of Macroscopic Binary Systems*

G. G. Adamian,N. V. Antonenko,H. Lenske,V. V. Sargsyan

Fig. 4 The calculated dimensionless relative distance $R_{m}^{d}$ (a) and orbital rotation period $ P_{\rm orb}^{d}$ (b) as functions of mass asymmetry in the cases of antiparallel spins with $L_1=J_{\rm tot}+S_1-S_2$ (dashed line) and $L_2=J_{\rm tot}-S_1+S_2$ (solid line), $n=3$, and $R_{m}>R_{t}=R_1+R_2$.