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Table 3.
Summary of the noteworthy characteristics of the new Li-rich giants as discussed in Sects. 3 and 4.
| CNAME | Characteristics |
|---|---|
| 08405643–5308309 | Above the bump in both the T eff–log g diagram (Fig. 2) and the HR-diagram (Fig. 7); bottom left panels. |
| 17522490–2927512 | |
| 17531013–2932063 | [α/Fe] > +0.15 |
| 18181062–3246291 | |
| 18182698–3242584 | α-enhanced with super-solar metallicity. |
| 18265248+0627259 | Possible core-He burning intermediate-mass giant? (bottom left panel of Fig. 2); candidate for planet engulfment (fast rotation); closer to the clump in the HR-diagram (Fig. 7). |
| 19223053+0138518 | |
| 19251759+0053140 | |
| 19261134+0051569 | S/N < 30; [α/Fe] > +0.15 |
| 19263808+0054441 | |
| 19264134+0137595 | |
| 19264917–0027469 | Above the bump (T eff–log g diagram, bottom-middle panel of Fig. 2); S/N < 30; [α/Fe] > +0.15; luminosity not computed. |
| 19265013+0149070 | [α/Fe] > +0.15; Ba enhanced (mass transfer from an AGB?). |
| 19265193+0044004 | Core-He burning giant from seismic data. |
| 19270600+0134446 | Infrared excess at 22 μm. |
| 19270815+0017461 | Above the bump (T eff–log g diagram, bottom left panel of Fig. 2); S/N < 30; [α/Fe] > +0.15; luminosity not computed. |
| 19273856+0024149 | Above the bump (T eff–log g diagram, bottom left panel of Fig. 2); S/N < 30; [α/Fe] > +0.15; luminosity not computed. |
| 19274706+0023447 | Below the bump (T eff–log g diagram, top middle panel of Fig. 2); S/N < 30; candidate for planet engulfment (fast rotation); at the clump in the HR-diagram (top middle panel of Fig. 7). |
| 19280508+0100139 | |
| 19283226+0033072 |
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