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Table 1.
Characteristics of the models used in this study.
| Model name | Xint | Xext | Rdisc/Req |  |
 |
EOS | Opacities |
|---|---|---|---|---|---|---|---|
| Mreal | 0.70 | 0.70 | n.a. | 1 | 1 | OPAL | OPAL |
| M | 0.70 | 0.70 | n.a. | 1 | 1 | Ideal gas | Kramer |
| M6 | 0.07 | 0.70 | 0.857074 | 0.513889 | 1.394972 | Ideal gas | Kramer |
| M7 | 0.07 | 0.70 | 0.962678 | 0.513889 | 1.394972 | Ideal gas | Kramer |
| M7b | 0.70 | 0.07 | 0.991861 | 1.945946 | 0.716860 | Ideal gas | Kramer |
Notes. Xint and Xext are the hydrogen contents below and above the discontinuity, respectively. Rdisc/Req gives the equatorial radius at the discontinuity, normalised by the star’s equatorial radius. We note that models Mreal and M are smooth.
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