Table 10: Time development of orbital variability in binary systems with observed giant planets.
Binary 1 K 10 K 100 K 150 K

system [%] [%] [%] [%]

$\tau$ Boo 0.283994 0.284011 0.284353 0.283526

HD 195019 0.334530 0.334614 0.335292 0.335452

GJ 86 0.469386 0.469395 0.470148 0.471522

**Table 10:** Time development of orbital variability in binary systems with observed giant planets.
Binary	1 K	10 K	100 K	150 K
system	[%]	[%]	[%]	[%]
$\tau$ Boo	0.283994	0.284011	0.284353	0.283526
HD 195019	0.334530	0.334614	0.335292	0.335452
GJ 86	0.469386	0.469395	0.470148	0.471522

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