Table 6
Li-rich stars discovered in M30.
| ID | RA | Dec | V | V−I | M V | Teff | log g | [Fe/H] | A(Li) | Ref. |
| # | (J2000) | (J2000) | [K] | [cm s-2] | [dex] | [dex] | ||||
|
|
||||||||||
| 1966 | 21 40 09.52 | −23 09 46.6 | 17.739 | 0.806 | 3.01 | 5487 | 3.46 |
−2.45
a
|
2.39 ± 0.07 | this work |
| M30-132 | 21 40 09.50 | −23 09 46.4 | 17.60 | 0.72 | 3.04 | 5640 | 3.54 | −2.43 ± 0.12 | 2.66 ± 0.14 | K16b |
| M30-7229 | 21 40 18.77 | −23 13 40.4 | 17.05 | 0.75 | 2.49 | 5510 | 3.28 | −2.32 ± 0.11 | 2.87 ± 0.13 | K16b |
Notes. The ids for the Kirby et al. (2016) stars refer to the Sandquist et al. (1999) catalogue. Crossmatching our catalogue with the Sandquist et al. (1999) catalogue identified stars M30-132 and 1966 as the same.
As a result of the limiting signal-to-noise ratio of the stellar spectrum only an upper estimate for the Fe abundance could be derived.
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