Table 12.
Effective temperature, surface gravity, mass, and apparent visual magnitude values of the stars showing pulsational light variations.
| Star | Teff [K] | log g [dex] | M* [M⊙] | mV [mag] |
|---|---|---|---|---|
| Ross 548 | 12 300G | 8.03 | 0.63 | 14.148 ± 0.03 |
| EC 23487-2424 | 11 560G | 8.09 | 0.66 | 15.256 ± 0.01 |
| BPM 31594 | 11 500G | 8.05 | 0.64 | 14.913 ± 0.11 |
| BPM 30551 | 11 240G | 8.16 | 0.70 | 15.394 |
| MCT 0145-2211 | 11 850G | 8.15 | 0.70 | 15.150 ± 0.07 |
| L 19-2 | 12 070G | 8.13 | 0.69 | 13.351 ± 0.03 |
| HS 1013+0321 | 11 630T | 8.12 | 0.68 | 15.585 ± 0.10 |
Notes. The superscripts G and T denote the original sources of the effective temperature and surface gravity values. In the case of the errors determined by Gianninas et al. (2011), these are around 200 K and 0.04 − 0.05 dex for the Teff and log g values, respectively, which means about 0.03 M⊙ errors for the stellar masses. In the only case when the source of the atmospheric parameters was Tremblay et al. (2011), the corresponding errors are 40 K and 0.01 dex.
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