Table 6: Dependence of orbital stability on simulation time.
Binary $R_{\rm AG}$ Orbital Orbital
system [AU] periods stability
2 22.325 10 MS
  22.325 20 U
  22.350 10 MS
  22.350 20 MS
  22.350 30 MS
  22.350 40 MS
  22.350 50 U
  22.500 101 MS
  22.500 102 MS
  22.500 103 MS
  22.500 104 MS
  22.500 105 U
Note: Simulations were performed for giant
planets with $M_{\rm G}$ = 1  $M_{\rm Jup}$.

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