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Table C.1.
Adopted parameters for notional main sequence secondary stars, we assume log g = 4.25 for all models. We also list the resulting effective equivalent width for the Mg II 4481 Å line in the combined spectrum. Estimates of the approximate stellar mass are given for two isochrones; 106 yrs and 107.5 yrs.
| Spectral | Teff | MV | EW | Mass (M⊙) | |
|---|---|---|---|---|---|
| type | K | mag | (mÅ) | 6.0 | 7.5 |
| B2 V | 21500 | −1.7 | 30 | 8.8 | 6.9 |
| B2.5 V | 20000 | −1.1 | 20 | 7.0 | 6.1 |
| B3 V | 16500 | −0.6 | 15 | 5.9 | 5.3 |
| B5 V | 15000 | +0.3 | 8.6 | 4.0 | 3.7 |
| B8 V | 13500 | +0.6 | 6.0 | 3.4 | 3.2 |
| B9 V | 12000 | +1.2 | 3.4 | 2.5 | 2.5 |
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