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Table 1

Parameter setup of each simulation A through U.

Simulation Binary system h α Σ0 (M/au2) Self-gravity Boundary α Σ

A Kepler-16 0.03 10-3 1.0 × 10-4 No Rigid 1.5
B Kepler-16 0.05 10-3 1.0 × 10-4 No Rigid 1.5
C Kepler-16 0.03 10-2 1.0 × 10-4 No Rigid 1.5
D Kepler-16 0.05 10-2 1.0 × 10-4 No Rigid 1.5
E Kepler-34 0.03 10-3 1.0 × 10-4 No Rigid 1.5
F Kepler-34 0.05 10-3 1.0 × 10-4 No Rigid 1.5
G Kepler-34 0.03 10-2 1.0 × 10-4 No Rigid 1.5
H Kepler-34 0.05 10-2 1.0 × 10-4 No Rigid 1.5

I Kepler-16 0.03 10-3 1.0 × 10-4 Yes Rigid 1.5
J Kepler-16 0.05 10-3 1.0 × 10-4 Yes Rigid 1.5
K Kepler-34 0.03 10-3 1.0 × 10-4 Yes Rigid 1.5
L Kepler-34 0.05 10-3 1.0 × 10-4 Yes Rigid 1.5

M Kepler-16 0.05 10-3 1.0 × 10-4 No Open 1.5
N Kepler-34 0.05 10-3 1.0 × 10-4 No Open 1.5

O Kepler-16 0.05 10-3 5.0 × 10-4 Yes Rigid 1.5
P Kepler-16 0.05 10-3 1.0 × 10-3 Yes Rigid 1.5
Q Kepler-16 0.05 10-3 2.5 × 10-3 Yes Rigid 1.5
R Kepler-16 0.05 10-3 5.0 × 10-4 No Rigid 1.5
S Kepler-16 0.05 10-3 1.0 × 10-3 No Rigid 1.5
T Kepler-16 0.05 10-3 2.5 × 10-3 No Rigid 1.5

U Kepler-16 0.05 10-3 1.0 × 10-4 Yes Rigid 0.5

Notes. AH test the effect of varying aspect ratio, alpha-viscosity and central binary type on non self-gravitating disks. IL test the inclusion of self-gravity at standard surface density. MN investigate the inclusion of an open boundary. OT look at the relevance of self-gravity in more detail by increasing the surface density of the disk. U tests the dependency of the disk evolution on the surface density profile exponent, αΣ.

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