Table 3.

Instability mass ratio for systems with primary stars of |$0.5\, \mathrm{M}_{\odot }\lt M\lt 1.6\,\mathrm{M}_{\odot }$| and various fill-out fractions. qinst as M2/M1.

Massqinstqinstqinstqinstqinstqinst
(M)f=1.0f=0.9f=0.75f=0.5f=0.25f=0
0.50.2530.2460.2360.2200.2070.196
0.60.2130.2080.2000.1890.1780.169
0.70.1820.1780.1720.1630.1550.148
0.80.1600.1560.1520.1450.1380.132
0.90.1360.1340.1300.1250.1200.115
1.00.1260.1240.1210.1160.1110.107
1.20.0870.0860.0840.0810.0790.076
1.40.0540.0530.0520.0510.0500.049
1.60.0470.0460.0460.0450.0440.043
Massqinstqinstqinstqinstqinstqinst
(M)f=1.0f=0.9f=0.75f=0.5f=0.25f=0
0.50.2530.2460.2360.2200.2070.196
0.60.2130.2080.2000.1890.1780.169
0.70.1820.1780.1720.1630.1550.148
0.80.1600.1560.1520.1450.1380.132
0.90.1360.1340.1300.1250.1200.115
1.00.1260.1240.1210.1160.1110.107
1.20.0870.0860.0840.0810.0790.076
1.40.0540.0530.0520.0510.0500.049
1.60.0470.0460.0460.0450.0440.043
Table 3.

Instability mass ratio for systems with primary stars of |$0.5\, \mathrm{M}_{\odot }\lt M\lt 1.6\,\mathrm{M}_{\odot }$| and various fill-out fractions. qinst as M2/M1.

Massqinstqinstqinstqinstqinstqinst
(M)f=1.0f=0.9f=0.75f=0.5f=0.25f=0
0.50.2530.2460.2360.2200.2070.196
0.60.2130.2080.2000.1890.1780.169
0.70.1820.1780.1720.1630.1550.148
0.80.1600.1560.1520.1450.1380.132
0.90.1360.1340.1300.1250.1200.115
1.00.1260.1240.1210.1160.1110.107
1.20.0870.0860.0840.0810.0790.076
1.40.0540.0530.0520.0510.0500.049
1.60.0470.0460.0460.0450.0440.043
Massqinstqinstqinstqinstqinstqinst
(M)f=1.0f=0.9f=0.75f=0.5f=0.25f=0
0.50.2530.2460.2360.2200.2070.196
0.60.2130.2080.2000.1890.1780.169
0.70.1820.1780.1720.1630.1550.148
0.80.1600.1560.1520.1450.1380.132
0.90.1360.1340.1300.1250.1200.115
1.00.1260.1240.1210.1160.1110.107
1.20.0870.0860.0840.0810.0790.076
1.40.0540.0530.0520.0510.0500.049
1.60.0470.0460.0460.0450.0440.043
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