Table 1
Li abundances and the chromospheric activity index (log 
) for 14 active stars.
| # | Stars | SpT. | V | B − V | log g | Teff | EW(Li) | log N(Li) | Prot | RO | log( ) |
|---|---|---|---|---|---|---|---|---|---|---|---|
| (mag) | (K) | (mÅ) | |||||||||
| 1 | [LH98] 17 | K2IV | 10.59 | 0.985 | 4.35 | 4867 | 169 | 2.26 | 7.9809(N) | 0.105 | –4.340(Wh) |
| 2 | HD 23386 | G0V | 9.56 | 0.693 | 4.5 | 5660 | 203 | 3.18 | 1.5775(B) | 0.021 | –3.970(Ma) |
| 3 | HD 282346 | G8V | 9.71 | 0.789 | 4.07 | 5309 | 218 | 2.81 | 0.7333(M) | 0.014 | –4.270(Wh) |
| 4 | HD 220140 | G9V | 7.54 | 0.893 | 4.6 | 5144 | 198 | 2.29 | 2.7(K) | 0.042 | –4.030(H) |
| 5 | HD 141004 | G0V | 4.42 | 0.600 | 4.3 | 6016 | 15 | 1.91 | 19(Is) | 0.685 | –4.970(Rad) |
| 6 | HD 101501 | G8V | 5.34 | 0.723 | 4.43 | 5488 | 26 | 0.84 | 11(Is) | 0.334 | –4.530(Rad) |
| 7 | HD 133640 | G0V | 4.85 | 0.647 | 4.33 | 5855 | 30.2 | 2.14 | 6.43(Rag) | 0.185 | –4.637(Ma) |
| 8 | BD+21 418 | G5 | 8.51 | 0.710 | 4.44 | 5752 | 153 | 3.20 | 6(Is) | 0.123 | –4.377(Is) |
| 9 | HD 26923 | G0IV | 6.5 | 0.56 | 4.13 | 6031 | 87 | 2.70 | 7(Ba) | 0.297 | –4.500(Ma) |
| 10 | HD 35984 | F6III | 6.19 | 0.476 | 4.2 | 6939 | 45 | 2.61 | 2.6(Ru) | 0.186 | –4.064(Bor) |
| 11 | HD 90709 | G5 | 7.04 | 0.789 | 4.84 | 5109 | 23.2 | 1.5 | 10(Is) | 0.180 | –4.419(Is) |
| 12 | HD 82443 | K0V | 7.01 | 0.779 | 4.43 | 5324 | 175 | 2.59 | 6(Ba) | 0.110 | –4.211(Ba) |
| 13 | HD 111395 | G5V | 6.31 | 0.703 | 4.55 | 5508 | 30.8 | 1.36 | 13(Is) | 0.355 | –4.66 (Br) |
| 14 | HD 141272 | K0V | 7.422 | 0.801 | 4.34 | 5279 | 16.9 | 0.86 | 11(Is) | 0.194 | –4.447(Mi) |
References. (N)Norton et al. (2007); (B)Bouvier et al. (2018); (By)Byrne et al. (1984); (K)Kahanpaeae et al. (1999); (Is)Isaacson & Fischer (2010); (Rag)Raghavan et al. (2010); (Ba)Baliunas et al. (1996); (Ru)Rutten (1987); (Wh)White et al. (2007); (Ma)Mamajek & Hillenbrand (2008); (Ga)Gagné et al. (2016); (Mi)Mishenina et al. (2012); (H)Herrero et al. (2012); (Rad)Radick et al. (2018); (Bor)Boro et al. (2018); (Ba)Baliunas et al. (1996); (Br)Brewer et al. (2016).
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