Table 2.
Physical properties for the seven RGB stars for which Miglio et al. (2016) reported unequivocal solar-like oscillations.
| ID | Δν | νmax | Teff [K] | Teff [K] |
|---|---|---|---|---|
| [μHz] | [μHz] | ±100 K | ±150 K | |
| Miglio et al. (2016) | This work | |||
| S1 | 1.83 ± 0.02 | 11.1 ± 0.4 | 4585 | 4671 |
| S2 | 2.55 ± 0.04 | 17.2 ± 0.7 | 4715 | 4767 |
| S3 | 2.62 ± 0.04 | 17.7 ± 0.7 | 4710 | 4815 |
| S4 | 2.64 ± 0.02 | 18.5 ± 0.7 | 4715 | 4801 |
| S5 | 4.14 ± 0.02 | 32.5 ± 1.3 | 4847 | 4964 |
| S6 | 4.30 ± 0.02 | 32.9 ± 1.3 | 4842 | 4976 |
| S7 | 4.30 ± 0.02 | 34.3 ± 1.4 | 4805 | 4915 |
Notes. The first column reports the ID used in Miglio et al. (2016) to identify the seven RGB stars. The second, third, and fourth columns show the global seismic parameters and the effective temperatures from Miglio et al. (2016). The effective temperatures computed in this work are shown in the last column.
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