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Table A.1
Abundances of the elements per million hydrogen atoms and their plausible main carriers in the dust phase of the local interstellar cloud (LIC).
| Element | Compound | Dust | Gas | Sun | |||||
|---|---|---|---|---|---|---|---|---|---|
| MgAl2O4 | FeNi | Mg2SiO4 | MgSiO3 | FeS | CHON | ||||
| C | 0 | 0 | 0 | 0 | 0 |  |
 |
 |
 |
| N | 0 | 0 | 0 | 0 | 0 |  |
 |
 |
 |
| O |  |
0 |  |
 |
0 |  |
 |
 |
 |
| Mg |  |
0 |  |
 |
0 | 0 |  |
 |
 |
| Al |  |
0 | 0 | 0 | 0 | 0 |  |
 |
 |
| Si | 0 | 0 |  |
 |
0 | 0 |  |
 |
 |
| S | 0 | 0 | 0 | 0 |  |
0 |  |
 |
 |
| Fe | 0 |  |
0 | 0 |  |
0 |  |
 |
 |
Notes. The solar and gas-phase abundances of elements are taken from Asplund et al. (2009) and Kimura et al. (2003b), respectively.
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