Table 7
Binary system parameters for two orbital inclinations.
| i = 90° | i = 48.5° | |||||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| q | M1 (M⊙) | M2 (M⊙) | a (R⊙) | R1 (R⊙) | Mbol 1 (mag) | R2 (R⊙) | Mbol 2 (mag) | M1 (M⊙) | M2 (M⊙) | a (R⊙) | R1 (R⊙) | Mbol 1 (mag) | R2 (R⊙) | Mbol 2 (mag) |
| 0.9 | 6.7 | 6.0 | 223 | 86.5 | −5.7 | 12.1 | −7.5 | 16.0 | 14.4 | 297 | 115.5 | −6.3 | 16.1 | −8.1 |
| 1.0 | 5.4 | 5.4 | 211 | 80.0 | −5.5 | 11.2 | −7.3 | 12.9 | 12.9 | 281 | 106.0 | −6.1 | 15.0 | −7.9 |
| 1.25 | 3.5 | 4.4 | 190 | 68.3 | −5.2 | 9.6 | −7.0 | 8.4 | 10.5 | 254 | 91.2 | −5.8 | 12.8 | −7.6 |
| 1.5 | 2.5 | 3.8 | 176 | 60.6 | −4.9 | 8.5 | −6.7 | 6.0 | 9.0 | 235 | 80.9 | −5.5 | 11.3 | −7.3 |
| 2.0 | 1.5 | 3.0 | 158 | 50.8 | −4.5 | 7.1 | −6.3 | 3.6 | 7.3 | 211 | 67.8 | −5.2 | 9.5 | −7.0 |
Notes. The Table describes the stellar masses (M1 and M2), orbital separation (a), stellar radii (R1 and R2), and bolometric magnitudes (Mbol 1 and Mbol 2) of the binary components for two different orbital inclinations. The stellar radii represent the upper limit corresponding to the case in which the donor star fills its Roche lobe, 
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