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Table 3
Predicted surface composition from a scaled-solar 1.5 M⊙, Z = 0.001 star model at the tip of the AGB.
| A(C) | A(N) | A(O) | A(F) | [F/O] | [Y/Fe] | [Zr/Fe] | [Ba/Fe] | [Nd/Fe] | [Pb/Fe] | |
|
|
||||||||||
| Initial | 7.29 | 6.69 | 7.55 | 3.24 | 0.00 | 0.00 | 0.00 | 0.00 | 0.00 | 0.00 |
|
|
||||||||||
| 0.002 | 8.91 | 7.17 | 7.79 | 4.81 | 1.32 | 1.11 | 1.21 | 1.70 | 1.71 | 2.61 |
| 0.0004 | 8.94 | 7.17 | 7.74 | 4.59 | 1.16 | 0.51 | 0.60 | 1.05 | 1.07 | 1.96 |
Notes. The [Fe/H] of the model star is − 1.18, and initial abundances are given in the first row.The [F/O] and [X/Fe] abundances ratios were normalized to the solar abundances from Asplund et al. (2009).
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