Table 9: Stability of S-type orbits in binary systems with observed giant planets.
Binary $M_{\rm A}$ $M_{\rm B}$ $M_{\rm B} / M_{\rm A}$ $M_{\rm G}$ $R_{\rm AB}$ $R_{\rm AG}$ $R_{\rm AG}/R_{\rm AB}$ Orbital

system [ $M_\odot$ ] [ $M_\odot$ ] [ $M_{\rm Jup}$ ] [AU] [AU] stability

$\tau$ Boo 1.3 0.4 0.3 3.87 225 0.0462 $2.1 \times 10^{-4}$ S

HD 195019 1.0 0.7 0.7 3.51 157 0.14 $8.9 \times 10^{-4}$ S

GJ 86 0.8 0.05 0.06 4.00 20 0.11 $5.5 \times 10^{-3}$ S

**Table 9:** Stability of S-type orbits in binary systems with observed giant planets.
Binary	$M_{\rm A}$	$M_{\rm B}$	$M_{\rm B} / M_{\rm A}$	$M_{\rm G}$	$R_{\rm AB}$	$R_{\rm AG}$	$R_{\rm AG}/R_{\rm AB}$	Orbital
system	[ $M_\odot$ ]	[ $M_\odot$ ]		[ $M_{\rm Jup}$ ]	[AU]	[AU]		stability
$\tau$ Boo	1.3	0.4	0.3	3.87	225	0.0462	$2.1 \times 10^{-4}$	S
HD 195019	1.0	0.7	0.7	3.51	157	0.14	$8.9 \times 10^{-4}$	S
GJ 86	0.8	0.05	0.06	4.00	20	0.11	$5.5 \times 10^{-3}$	S

Source LaTeX | All tables | In the text

	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