Table A.1
Elemental abundances (in mole) in stars selected for this sample study.
| Star | C | O | Mg | Ni | Si | S | Ti | Fe |
|
|
||||||||
| Sun | 2.88 × 108 | 5.75 × 108 | 4.17 × 107 | 1.95 × 106 | 4.07 × 107 | 1.82 × 107 | 1.00 × 105 | 3.47 × 107 |
| 55 Cancri | 7.40 × 108 | 7.40 × 108 | 1.20 × 108 | 3.60 × 106 | 6.90 × 107 | 2.10 × 107 | 2.20 × 105 | 6.30 × 107 |
| HD 967 | 1.45 × 108 | 5.75 × 108 | 1.70 × 107 | 3.98 × 105 | 1.26 × 107 | − | 4.17 × 104 | 9.77 × 106 |
| HD 1581 | 2.29 × 108 | 5.37 × 108 | 2.88 × 107 | 1.12 × 106 | 2.57 × 107 | − | 7.41 × 104 | 3.09 × 107 |
| HD 2071 | 2.75 × 108 | 5.75 × 108 | 3.16 × 107 | 1.38 × 106 | 2.95 × 107 | − | 8.71 × 104 | 3.80 × 107 |
| HD 4308 | 2.63 × 108 | 6.76 × 108 | 3.16 × 107 | 8.91 × 105 | 2.40 × 107 | − | 7.59 × 104 | 2.14 × 107 |
| HD 6348 | 1.91 × 108 | 3.80 × 108 | 1.48 × 107 | 4.57 × 105 | 1.20 × 107 | − | 4.68 × 104 | 1.29 × 107 |
| HD 9826 | 4.79 × 108 | 7.59 × 108 | 6.38 × 107 | 2.37 × 106 | 5.42 × 107 | 1.74 × 107 | 1.35 × 105 | 4.69 × 107 |
| HD 19034 | 2.24 × 108 | 6.92 × 108 | 2.75 × 107 | 6.31 × 105 | 1.91 × 107 | − | 6.61 × 104 | 1.55 × 107 |
| HD 37124 | 2.46 × 108 | 5.96 × 108 | 3.24 × 107 | 7.41 × 105 | 1.91 × 107 | 5.25 × 106 | 7.00 × 104 | 1.29 × 107 |
| HD 66428 | 6.31 × 108 | 1.05 × 109 | 1.48 × 108 | 3.72 × 106 | 6.92 × 107 | − | 1.78 × 105 | 8.32 × 107 |
| HD 95128 | 3.84 × 108 | 7.10 × 108 | 4.27 × 107 | 1.86 × 106 | 4.27 × 107 | 1.45 × 107 | 1.14 × 105 | 3.72 × 107 |
| HD 142022 | 4.90 × 108 | 8.20 × 108 | 9.12 × 107 | 2.82 × 106 | 5.62 × 107 | − | 1.70 × 105 | 7.24 × 107 |
| HD 147513 | 2.40 × 108 | 1.51 × 109 | 3.47 × 107 | 2.19 × 106 | 4.57 × 107 | − | 1.62 × 105 | 5.01 × 107 |
| HD 160691 | 5.25 × 108 | 7.08 × 108 | 8.51 × 107 | 4.37 × 106 | 8.32 × 107 | 2.57 × 107 | 2.07 × 105 | 7.08 × 107 |
| HD 213240 | 5.40 × 108 | 1.20 × 109 | 6.50 × 107 | 2.40 × 106 | 4.40 × 107 | 1.30 × 107 | 1.30 × 105 | 4.40 × 107 |
| HD 220367 | 2.40 × 108 | 5.89 × 108 | 3.80 × 107 | 1.05 × 106 | 2.45 × 107 | − | 7.08 × 104 | 2.88 × 107 |
| HD 221287 | 3.09 × 108 | 9.77 × 108 | 3.16 × 107 | 1.70 × 106 | 3.63 × 107 | − | 1.12 × 105 | 5.13 × 107 |
| Star | N | Na | Al | P | Ca | Cr | Reference | |
| Sun | 7.94 × 107 | 2.34 × 106 | 3.47 × 106 | 3.47 × 105 | 2.57 × 106 | 5.25 × 105 | 1 | |
| 55 Cancri | 1.80 × 108 | 3.90 × 106 | 8.70 × 106 | 8.50 × 105 | 2.80 × 106 | 7.80 × 105 | 2, 3, 4, 5 | |
| HD 967 | − | 5.50 × 105 | 1.23 × 106 | − | 7.94 × 105 | 1.20 × 105 | 6, 7, 8 | |
| HD 1581 | − | 1.38 × 106 | 1.95 × 106 | − | 1.70 × 106 | 3.31 × 105 | 6, 7, 8 | |
| HD 2071 | − | 1.66 × 106 | 2.45 × 106 | − | 1.95 × 106 | 3.63 × 105 | 6, 7, 8 | |
| HD 4308 | − | 1.17 × 106 | 2.45 × 106 | − | 1.48 × 106 | 2.14 × 105 | 6, 7, 8 | |
| HD 6348 | − | 5.37 × 105 | 1.17 × 106 | − | 7.94 × 105 | 1.48 × 105 | 6, 7, 8 | |
| HD 9826 | 8.51 × 107 | 3.94 × 106 | − | − | 3.10 × 106 | − | 9, 11, 12 | |
| HD 19034 | − | 9.12 × 105 | 2.04 × 106 | − | 1.20 × 106 | 1.78 × 105 | 6, 7, 8 | |
| HD 37124 | − | 9.33 × 105 | 2.29 × 106 | − | 1.15 × 106 | 1.70 × 105 | 9, 10, 11 | |
| HD 66428 | − | 4.90 × 106 | 6.31 × 106 | − | 3.72 × 106 | 8.32 × 105 | 6, 7, 8 | |
| HD 95128 | 1.05 × 108 | 2.40 × 106 | 3.47 × 106 | − | 2.24 × 106 | 4.90 × 105 | 9, 10, 11, 12 | |
| HD 142022 | − | 2.82 × 106 | 5.13 × 106 | − | 3.39 × 106 | 6.76 × 105 | 6, 7, 8 | |
| HD 147513 | − | 1.95 × 106 | 3.31 × 106 | − | 3.31 × 106 | 4.90 × 105 | 6, 7, 8 | |
| HD 160691 | − | 5.50 × 106 | 7.59 × 106 | − | 4.47 × 106 | 1.01 × 106 | 2, 9, 11, 13 | |
| HD 213240 | 1.40 × 107 | 3.60 × 106 | 4.70 × 106 | 4.60 × 105 | 2.50 × 106 | 5.20 × 105 | 2, 3, 4, 5 | |
| HD 220367 | − | 1.29 × 106 | 2.40 × 106 | − | 1.55 × 106 | 2.88 × 105 | 6, 7, 8 | |
| HD 221287 | − | 1.86 × 106 | 2.40 × 106 | − | 2.63 × 106 | 5.01 × 105 | 6, 7, 8 | |
Notes. The abundances of all elements in all stars are reported relative to an H abundance of 1 × 1012 mole. When no values were found for an element, the solar elemental abundances were taken for the calculations.
Reference. 1) Lodders (2003); 2) Gilli et al. (2006); 3) Beirão et al. (2005); 4) Ecuvillon et al. (2004); 5) Ecuvillon et al. (2006); 6) Delgado Mena et al. (2010); 7) Neves et al. (2009); 8) Sousa et al. (2008); 9) Gonzalez & Laws (2007); 10) Kang et al. (2011); 11) Caffau et al. (2005); 12) Takeda & Honda (2005); 13) Morel & Micela (2004).
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