Table 3.
Main parameters of the known MW Li-rich DCEPs.
| Star | D | AV | Teff | L | A(Li) | [Fe/H] |
|---|---|---|---|---|---|---|
| (pc) | (mag) | (K) | (L⊙) | (dex) | (dex) | |
| ASAS J075842–2536.1 | 2601 ± 115 | 0.939 | 6295 | 145 ± 14 | 2.84 ± 0.10 | −0.16 ± 0.12 |
| ASAS J131714–6605.0 | 2746 ± 92 | 1.686 | 6308 | 524 ± 35 | 2.96 ± 0.10 | 0.05 ± 0.06 |
| V371 Per | 3255 ± 129 | 0.319 | 5973 | 474 ± 39 | 3.09 ± 0.10 | −0.46 ± 0.09 |
| V1033 Cyg | 3621 ± 374 | 2.478 | 5819 | 911 ± 190 | 3.18 ± 0.10 | 0.01 ± 0.11 |
| V363 Cas | 1215 ± 16 | 1.545 | 6660 | 287 ± 8 | 2.86 ± 0.10 | −0.30 ± 0.12 |
Notes. Distances are from Bailer-Jones et al. (2021), extinctions from Anders et al. (2019), and effective temperatures and lithium and iron abundances are from Kovtyukh et al. (2019) for all the stars except for V363 Cas taken from Catanzaro et al. (2020). Luminosities have been computed using VOSA tools.
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