over-enhancements of the neutron-capture elements cannot change the lighter elements away from the standard halo patterns. \[Cu/Fe\] and \[Zn/Fe\] in CS 31062-050 agree with the trends seen in the majority of metal-poor stars (Sneden, Gratton, & Crocker 1991; Primas [et al.]{} 2000).

[lrrrrcr]{} & 6.01 & 0.84 & 0.20 & 0.21 & 1 &\
& 4.43 & 0.49 & 0.10 &0.09 & 2 &\
& 2.85 & 0.32 & 0.25 & 0.13 & 9 &\
& 2.86 & 0.33 & 0.10 & 0.23 & 4 &\
& 1.44 & $-$0.17& 0.14 &0.18 & 2 &\
& 3.36 &0.08 & 0.19 & 0.15 & 3 &\
& 2.69 & $-$0.43& 0.12 &0.12 & 4 &\
& 5.09 & $-$2.41 & 0.11 &0.13 & 46 & $-$0.10\
& 5.10 & $-$2.40 &0.13 &0.15 &10 & $-$0.07\
& 2.60 & 0.10 & 0.20 & 0.23& 1 &\
& 3.68 & $-$0.16 & 0.17 & 0.21 & 11 &\
& 0.69 & $-$1.19& 0.20 & 0.18 & 2 &\
& 2.32 & 0.06 & 0.20 & 0.23 & 1 &\
& 0.30 & 0.48 &0.10 & 0.22 & 14 &\
& 1.05 & 0.85 & 0.14 & 0.19 &9 & $-$0.26\
& 0.27 & 