Table 1
Elemental atomic abundances used in GGCHEM for solar composition and the sulfur-rich composition associated with HIP 43393.
| Elem. | Solar | HIP 43393 | Elem. | Solar | HIP 43393 |
|---|---|---|---|---|---|
| H | 13.49 | 13.82 | He | 12.42 | 12.75 |
| Fe | 8.99 | 8.75 | C | 9.92 | 9.94 |
| O | 10.18 | 10.54 | Mg | 9.09 | 9.13 |
| Si | 9.00 | 9.00 | Ca | 7.83 | 7.72 |
| Ti | 6.44 | 6.56 | Li | 2.54 | 2.56 |
| N | 9.32 | 9.34 | F | 6.05 | 6.07 |
| Na | 7.73 | 7.60 | Al | 7.94 | 8.01 |
| P | 6.90 | 6.92 | Cl | 6.99 | 7.01 |
| K | 6.52 | 6.54 | V | 5.42 | 5.48 |
| Cr | 7.13 | 6.97 | Mn | 6.92 | 6.52 |
| Ni | 7.71 | 7.48 | Zr | 4.07 | 4.20 |
| S | 8.61 | 9.04 | W | 2.34 | 2.36 |
Notes. Abundances are given in log units and are normalized to silicon (log nSi = 9). Solar abundances are taken from Asplund et al. (2009), while the abundances of HIP 43393 are from the Hypatia catalog (Hinkel et al. 2014).
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