Table 2.
Solar abundances and depletion factors for all the models analyzed in this paper.
| Element | 12 + log (X/H)tot | δ(X) |
|---|---|---|
| C | 8.55 | −0.2 |
| N | 7.97 | – |
| O | 8.87 | −0.2 |
| S | 7.27 | −0.2 |
| Mg | 7.58 | −1.2 |
| Si | 7.55 | −0.9 |
| P | 5.57 | −0.5 |
| Cl | 5.27 | 0 |
| Ti | 4.93 | −2.3 |
| Mn | 5.53 | −1.2 |
| Fe | 7.51 | −1.5 |
| Zn | 4.65 | −0.35 |
Notes. The solar abundances and the median depletion factors of metals from the gas phase onto dust grains are set according to Savage & Sembach (1996). The depletion factors are in agreement with those estimated by Jenkins (2009) for a depletion strength F* = 0.5.
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