Table 3: Dependence of orbital stability on mass of secondary star.
Binary $M_{\rm B} / M_{\rm A}$ $R_{\rm AG}$ $R_{\rm AG}/R_{\rm AB}$ Orbital
system   [AU]   stability
3 0.20 2.56 0.32 S
  0.40 2.56 0.32 MS
  0.60 2.56 0.32 MS
  0.80 2.56 0.32 U
Note: Simulations were performed for giant planets
with $M_{\rm G}$ = 1  $M_{\rm Jup}$ based on 1000 orbits.

Source LaTeX | All tables | In the text

Article Contents
1 Introduction
2 Method and code testing
3 Initial conditions and stability criteria
4 Case studies
5 Binary systems with observed giant planets
6 Conclusions
References
List of tables
List of figures