Table A.14
Comparison of the sulphur abundances and ICFs used in this study with those in which ICFs from other sources have been applied (see Sect. 3.5.2).
| This work | B80 / KB94 | KH01 | DI14 | ||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|
| PN | S/H | α = 3 | α = 2 | S/H | S/H | ||||||
| × 10−6 | ICF(S) | S/H × 10−6 | ICF(S) | S/H × 10−6 | ICF(S) | × 10−6 | ICF(S) | × 10−6 | ICF(S) | ||
| K3-66 | 1.7 ± 0.6*†‡ | 1.18 | 1.4 ± 1.0*† | 1.10 | 1.6 ± 1.2*† | 1.29 | # | ... | # | ... | |
| K3-67 | 2.2 ± 0.7*†‡ | 1.18 | 2.1 ± 0.9*† | 1.98 | 3.6 ± 1.5*† | 3.38 | 1.2 ± 0.7*† | 1.22 | 1.9 ± 1.3*† | 1.91 | |
| K3-70 | 3.7 ± 1.8*†‡ | 1.18 | 3.3 ± 0.6*† | 1.33 | 4.5 ± 1.0*† | 1.79 | 2.7 ± 1.1*† | 1.09 | 3.3 ± 2.0*† | 1.31 | |
| K3-90 | 2.7 ± 1.2*†‡ | 1.18 | 3.6 ± 1.8*† | 5.39 | 10.1 ± 5.7*† | 15.3 | 1.9 ± 1.7*† | 2.86 | 12.4 ± 10.2*† | 18.7 | |
| K4-48 | 2.2 ± 0.7*†‡ | 1.18 | 2.3 ± 0.8*† | 1.51 | 3.3 ± 1.3*† | 2.20 | 1.7 ± 0.9*† | 1.13 | 2.3 ± 1.5*† | 1.52 | |
| M1-6 | 1.6 ± 0.6† | 1.11 | # | ... | # | ... | # | ... | # | ... | |
| M1-7 | 4.4 ± 2.6*†‡ | 1.18 | 3.6 ± 0.9*† | 1.21 | 4.6 ± 1.3*† | 1.53 | 3.2 ± 1.4*† | 1.07 | 3.4 ± 1.9*† | 1.15 | |
| M1-9 | 2.0 ± 1.0*†‡ | 1.00 | 2.2 ± 1.5*† | 1.21 | 2.9 ± 2.0*† | 1.53 | # | ... | # | ... | |
| M1-14 | 2.5 ± 1.0*†‡ | 1.00 | 2.7 ± 1.5*† | 1.14 | 3.3 ± 1.9*† | 1.39 | 2.6 ± 2.1*† | 1.06 | 2.6 ± 2.4*† | 1.04 | |
| M1-16 | 1.8 ± 0.9*†‡ | 1.18 | 1.7 ± 0.5*† | 1.37 | 2.3 ± 0.8*† | 1.90 | 1.3 ± 0.6*† | 1.10 | 1.7 ± 1.0*† | 1.38 | |
| M2-2 | 2.1 ± 0.5*†‡ | 1.18 | 1.3 ± 0.2*† | 2.47 | 2.5 ± 0.5*† | 4.72 | 0.72 ± 0.25*† | 1.35 | 1.2 ± 0.7*† | 2.28 | |
Notes. B80 = Barker (1980); KB94 = Kingsburgh & Barlow (1994); KH01 = Kwitter & Henry (2001); DI14 = Delgado-Inglada et al. (2014). In all cases, ICFs are applied to our sulphur ionic abundances from Table A.10. Superscript symbols show the ions considered in the calculations: * = S+; † = S2+; ‡ = S3+. # Uncertainties >100%, likely due to uncertainties in the ICF and S+ abundances given from Henry et al. (2010).
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