Table A.1
Adopted elemental abundances.
| X | I∕kB (a) | Y (X) | d(X) (b) |
|---|---|---|---|
| [K] | |||
| H | 157 803 | 12.00 | 1.0 |
| C | 130 670 | 8.43 | 0.458 |
| Na | 59636 | 6.24 | 0.36 |
| Mg | 88731 | 7.60 | 0.112 |
| Al | 69462 | 6.45 | 0.00179 |
| Si | 94596 | 7.51 | 0.0479 |
| P | 121 693 | 5.41 | 1.0 |
| S | 120 223 | 7.12 | 1.0 |
| Cl | 150 483 | 5.50 | 0.324 |
| K | 50371 | 5.03 | 0.078 |
| Ca | 70940 | 6.34 | 0.0001739 |
| Ti | 79237 | 4.95 | 0.0022 |
| Fe | 91704 | 7.50 | 0.00375 |
| Ni | 88657 | 6.22 | 0.00176 |
Notes. (a) The ionisation energy (kB is the Boltzmann constant). (b)The depletion factor. Solar photospheric abundances are taken from Asplund et al. (2009). Depleted abundances follow the patterns in diffuse molecular clouds and are taken from Draine (2011), except for Na and K (Lepp et al. 1988), P (Lebouteiller et al. 2005; James & Aloisi 2018), and Cl (Moomey et al. 2012).
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