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Table 4.
Main characteristics of the adopted asteroseismological models and of the ranges of possible solutions for the ELMVs shown in this work.
| Star | Teff (K) | log(g) (cgs) | M⋆ (M⊙) | log(MH/M⋆) | log(R⋆/R⊙) | log(L⋆/L⊙) |
|---|---|---|---|---|---|---|
| J1112* | 9301 | 5.9695 | 0.1612 | −1.76 | −1.1623 | −1.4932 |
| J1518 | 9487 | 6.9994 | 0.2390 | −3.67 | −1.5916 | −2.3200 |
| J1738 | (8883,9273) | (6.0506,6.6923) | (0.1612,0.1921) | (−5.43,−1.76) | (−1.5057,−1.2029) | (−2.2548,−1.6560) |
| J1735* | 8075 | 6.2241 | 0.1612 | −1.76 | −1.2899 | −1.9957 |
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