Table 8.
Seismic estimates of the surface gravity and stellar masses of the Li-rich giants in the CoRoT fields.
CNAME | CoRoT ID | log g | σlog g | Mass M⊙ | σmassM⊙ | Num. pipelines |
---|---|---|---|---|---|---|
19223053+0138518 | 100440565 | 2.35 | 0.05 | 1.25 | 0.14 | 4 |
19251759+0053140 | 100919702 | – | – | – | – | 0 |
19261134+0051569 | 101064590 | 2.34 | 0.07 | 2.75 | 1.37 | 1 |
19263808+0054441 | 101130864 | 2.48 | 0.02 | 0.91 | 0.12 | 2 |
19264134+0137595 | 101139596 | 2.39 | 0.07 | 1.55 | 0.19 | 3 |
19264917–0027469 | 101160340 | 1.93 | 0.06 | 1.46 | 0.46 | 1 |
19265013+0149070 | 101162874 | – | – | – | – | 0 |
19265193+0044004 | 101167637 | 2.42 | 0.03 | 1.20 | 0.15 | 4 |
19270600+0134446 | 101205220 | 2.48 | 0.05 | 1.74 | 0.56 | 1 |
19270815+0017461 | 101210895 | 2.23 | 0.02 | 1.29 | 0.18 | 1 |
19273856+0024149 | 101292381 | 2.10 | 0.04 | 1.54 | 0.27 | 3 |
19274706+0023447 | 101314825 | – | – | – | – | 0 |
19280508+0100139 | 101351658 | 2.30 | 0.08 | 3.03 | 1.60 | 1 |
19283226+0033072 | 101411079 | – | – | – | – | 0 |
Notes. The error in log g takes into account the error in Teff. Moreover, it includes both the standard and systematic errors for the targets for which detection was made by more than one pipeline. For the targets with only one determination, this is only the internal error of the pipeline (and thus it underestimates the uncertainty). The error in the masses also takes into account the error in vmax, which is usually large. Moreover, we remark again that masses based on scaling relations need corrections that depend on the stellar parameters, as discussed in the text, and which were not applied here.
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