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Table 2
Possible steps in the physical processes of partial mixing and nuclear H- and He-burning in massive very low Z stars.
Steps | Acting physical processes | Main nuclear products | Stars and properties |
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0 | Absence of mixing | Initial composition | Low Z stars without C excess |
0+ | Core H-burning | 13C, 14N | Very low CNO, but N > C, O |
1 | Core He-burning | 12C, 16O, no N | Visible only in WC stars |
1+ | Advanced He-burning | 12C ↘, 16O, low 20Ne | Visible only in WO stars |
2 | Partial mixing 12C, 16O in H-burning shell | 12C, 13C, 14N, 16O | CEMP-no with [C/N] > 0, [O/N] > 0 |
2+ | Idem with advanced H-burning | Idem | CEMP-no with [C/N] < 0, [O/N] < 0 |
2Na | Idem from 1+ with the Ne-Na cycle | Idem, 20,21,22Ne, 23Na | CEMP-no, [C/N] > 0, [O/N] > 0, Na |
2+Na | Idem 2Na, advanced H-burning | Idem, 20,21,22Ne, 23Na | CEMP-no, [C/N] < 0, [O/N] < 0, Na |
3 | Partial mixing prod. (2, 2+) in He-burn. zone | 18O, 22Ne | CEMP-no, N ↘, O-strong, 22Ne |
3+ | Idem with advanced α captures | O, 20,22Ne, 25,26Mg, Sr, Y | CEMP-no, idem, Mg, s-elem.(1st peak) |
3++ | Idem with more 22Ne (α,n)25Mg captures | Idem, Ba weak | Low s-star, Mg,s-el. (1st, 2nd peak) |
The same above 3 cases from (2Na, 2Na+) | Same properties as in above cases | ||
−→ cases 3Na, 3+Na, 3++Na | with Na present | ||
4 | Part. mix. 3 in H-burn., CNO, Ne-Na | CNO, Ne, Na, | CEMP-no, N↗, Ne, Na, |
4+ | Part. mix. 3+ in H-burn., CNO, Ne-Na, Mg-Al | CNO, Ne, Na, Mg, Al | CEMP-no, Na, Mg, Al, s-el.(1st peak) |
4++ | Partial mixing of 3++, idem | Idem | Low s, Na, Mg, Al, s-el.(1st, 2nd peak) |
Notes. He should be enriched in all cases, except for step number 0. See text for more details.
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