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| He | C | N | O | Ne | Mg | Si | P | S | Cl | Ar | Fe | |
| BY NUMBER in log | ||||||||||||
| Best Stellar Model | -0.60 | -3.30 | -4.24 | -3.42 | -4.29 | -7.11 | -5.36 | -5.29 | -4.74 | |||
| Best Nebular Model | -0.92 | -3.10 | -4.00 | -3.40 | -4.00 | -4.95 | -4.90 | -5.35 | -7.00 | -5.80 | -7.40 | |
| LITERATURE NEBULAR ABUNDANCES (BY NUMBER in log) | ||||||||||||
| Sterling et al. (2007) Model A | -0.975 | -3.22 | -3.97 | -3.29 | -3.99 | -5.40 | -7.07 | -5.79 | ||||
| Sterling et al. (2007) Model B | -0.850 | -3.32 | -3.97 | -3.43 | -3.75 | -5.35 | -7.11 | -5.81 | ||||
| Pottasch et al. (2004) | -1.142 | -3.21 | -4.02 | -3.46 | -4.05 | -5.36 | -6.92 | -5.74 | ||||
| Henry et al. (2000) | -1.066 | -3.66 | -4.07 | -3.81 | -5.02 | |||||||
| Hyung et al. (1994) Model | -1.155 | -3.52 | -4.15 | -3.74 | -5.52 | -5.55 | -6.00 | -5.60 | -7.00 | -6.26 | ||
| Hyung et al. (1994) ICF | -1.155 | -3.57 | -4.08 | -3.67 | -4.22 | -5.16 | -5.56 | -7.11 | -5.72 | |||
| Aller et al. (1980) | -0.920 | -3.22 | -4.22 | -3.37 | -4.40 | -5.38 | -6.85 | -5.34 | ||||
| Aller & Czyzak (1983) | -1.030 | -3.21 | -4.13 | -3.36 | -4.13 | -5.38 | -7.06 | -5.64 | ||||
| Beck et al. (1981) | -4.12 | -5.21 | -5.74 | |||||||||
| Buerger (1973) | -0.796 | -3.70 | -4.40 | -3.60 | -4.50 | -5.00 | -6.82 | -5.30 | ||||
| Solar (Asplund et al. 2005) | -1.070 | -3.61 | -4.22 | -3.34 | -4.16 | -4.47 | -4.49 | -7.00 | -4.86 | -6.50 | -5.82 | -4.55 |
| BY MASS in log | ||||||||||||
| Best-fit stellar model | -0.30 | -2.52 | -3.40 | -2.52 | -3.15 | -5.92 | -4.16 | -3.99 | -3.30 | |||
| Best-fit nebular model | -0.49 | -2.20 | -3.03 | -2.37 | -2.88 | -3.75 | -3.63 | -4.02 | -5.63 | -4.37 | -5.83 | |
| Solar (Asplund et al. 2005) | -0.60 | -2.66 | -3.21 | -2.27 | -2.99 | -3.22 | -3.17 | -5.28 | -3.49 | -5.09 | -4.35 | -2.93 |
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