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Table 5.
Comparison between the main characteristics of the adopted asteroseismological models for every ELMV WD shown in this work with the results obtained in Calcaferro et al. (2017b).
| Star | Work | Teff (K) | log(g) (cgs) | M⋆ (M⊙) | log(MH/M⋆) | log(R⋆/R⊙) | log(L⋆/L⊙) |
|---|---|---|---|---|---|---|---|
| J1112 | This | 9301 | 5.9695 | 0.1612 | −1.76 | −1.1623 | −1.4932 |
| Previous | 9300 | 6.9215 | 0.2390 | −2.45 | −1.5528 | −2.2757 | |
| J1518 | This | 9487 | 6.9994 | 0.2390 | −3.67 | −1.5916 | −2.3200 |
| Previous | 9789 | 7.0956 | 0.2707 | −2.96 | −1.6126 | −2.3098 | |
| J1738 | This | (8883,9273) | (6.0506,6.6923) | (0.1612,0.1921) | (−5.43,−1.76) | (−1.5057,−1.2029) | (−2.2548,−1.6560) |
| Previous | 9177 | 7.6241 | 0.4352 | −3.21 | −1.7746 | −2.7447 |
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