Table 8: Comparison of NGC 330 analyses in this paper with those from Lennon et al. (2003,  L03), and Korn et al. (2000,  K00). In L03 and K00, NGC 330-002, -004 and -018 are labeled with Robertson (1974) identifications, which are A02, B37 and B30. Fe has been omitted from this comparison as the other analyses did not consider this element. Abundances are presented as [X] = 12 + $\log$ ([X/H]) in units of dex.
  NGC 330-002   NGC 330-004   NGC 330-018
  This paper L03   This paper L03   This paper K00
$T_{\rm eff}$ (K) 14 590 16 000   17 000 18 000   18 000 16 950
$\log {g}$ (cm s-2) 2.15 2.30   2.30 2.40   2.95 2.77
$\xi $ (km s-1) 16 8   16 10   5 6
C 7.09 6.91   6.84 6.71   7.17 7.30:
N 7.59 $\pm$ 0.33 7.71   7.83 $\pm$ 0.14 7.89   7.24 $\pm$ 0.26  
O 7.98 $\pm$ 0.49 8.14   7.86 $\pm$ 0.32 7.98   8.05 $\pm$ 0.37 8.25 $\pm$ 0.30
Mg 6.60 $\pm$ 0.23 6.69   6.73 $\pm$ 0.21 6.79   6.61 $\pm$ 0.18 6.85 $\pm$ 0.40
Si 6.82 $\pm$ 0.46 6.82   6.82 $\pm$ 0.39 7.12   6.80 $\pm$ 0.36 6.82 $\pm$ 0.30

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