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Table 2.
Physical parameters adopted for the SED of main sequence stars orbiting a BLAP.
| Spec. type | Teff(K) | log g | R(R⊙) | M(M⊙) | Archetypal |
|---|---|---|---|---|---|
| BLAP | 27718 | 4.51 | 0.62 | 0.469 | |
| A0 | 10800 | 4.15 | 2.50 | 3.20 | α CrB A |
| F0 | 7240 | 4.44 | 1.30 | 1.70 | γ Vir |
| G0 | 5920 | 4.44 | 1.05 | 1.10 | β Com |
| K0 | 5240 | 4.47 | 0.85 | 0.78 | 70 Oph A |
| M0 | 3800 | 4.80 | 0.51 | 0.60 | Lacaille 8760 |
Notes. For the latter, we adopted the values from one of our binary models. For main sequence companions, we used literature parameters for an archetypal spectral types (Zombeck 2007).
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