Table 7: Lithium abundances for the stars in IC 4651, computed with both spectroscopic (S) and photometric (P) values of $T_{{\rm eff}}$, assuming a reddening of E(b-y) = 0.091; we use the latter in our analysis. Asterisks indicate that W(Li) (in mÅ) refers to the unblended Li line.
Star T(S) T(P) W(Li) $\log~N$(Li)(S) $\log~N$(Li)(P)
E12 5000 5020 <5 <0.35 <0.38
E8 4900 4950 <5 <0.09 <0.23
E98 4900 4950 16 * 0.72 0.82
E60 4900 4930 9 * 0.42 0.53
E812 5000 4910 <5 <0.38 <0.21
E95 5800 5670 35 * 2.19 2.07
E3 6550 6550 9 1.64 1.64
E56 6500 6520 <10 <2.15 <2.16
E19 6500 6280 <5 <1.83 <1.66
E99 6800 6830 <10 <2.36 <2.38
E25 6900 6680 75 3.44 3.29
E5 7100 6930 76 3.59 3.47
T1228 6800 6770 58 3.20 3.18
E14 6800 6860 <5 <2.03 <2.07
E34 6850 6640 <5 <2.07 <1.92
E15 6850 6540 <6 <2.15 <1.93
E79 6650 6620 <5 <1.93 <1.91
E64 6650 6550 10 * 2.24 2.17
E86 6600 6459 10 * 2.20 2.13
T2105 6350 6138 67 * 3.02 2.84
E7 6300 6308 53 * 2.83 2.84
E45 6350 6103 47 * 2.80 2.59


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