Table 7: Li abundances, in the scale log A(H) = 12, for the BPA proposed members having EW $_{\rm Li} > 0$ in Table 6. Column 1: star identification; Col. 2: effective temperature, from $(V-I)_{\rm C}$ ; Col. 3: equivalent width of the resonance lithium line in mÅ; Col. 4: log of Li abundance.
IDENT $T_{\rm eff}$ EW A(Li)

(1) (2) (3) (4)

HD 203 6897. 87 3.36

HIP 10679 5988. 160 3.08

HD 14082 6368. 140 3.34

BD+30 397B 3544. 110 -0.49

AG Tri 4351. 220 1.46

BD+05 378 4100. 450 2.24

GJ 3305 3715. 120 -0.11

V1005 Ori 3816. 270 0.76

CD-57 1054 3860. 360 1.29

HD 35850 6406. 191 3.72

AO Men 4377. 420 2.58

HD 139084B 3310. 460 0.26

V343 Nor 5168. 292 3.08

V824 Ara 5383. 250 3.07

HD 155555C 3413. 20 -1.76

CD-54 7336 5036. 360 3.36

HD 161460 5304. 320 3.46

HD 164249 6597. 107 3.31

HD 164249B 3544. 70 -0.74

V4046 Sgr 4361. 440 2.65

GSC 7396-0759 3619. 200 0.09

HD 168210 5645. 290 3.65

CD-64 1208 4148. 490 2.52

TYC 9073-0762-1 3649. 332 0.73

TYC 7408-0054-1 3889. 492 2.03

PZ Tel 5344. 287 3.30

TYC 6872-1011-1 3850. 483 1.91

CD-26 13904 4602. 320 2.39

HD 181327 6597. 120 3.40

AU Mic 3649. 80 -0.47

HD 199143 6330. 150 3.40

AZ Cap 4197. 420 2.26

CP-72 2713 3921. 440 1.84

TX PsA 3316. 450 0.26

BD-13 6424 3715. 185 0.20