Table 2
Nucleosynthesis prescriptions.
| Model | Adopted stellar yields | Comments | |
| LIMSs | Massive stars | ||
|
|
|||
| 1 | vdHG97, ηAGB var | WW95, case B | Reference model |
| 2 | vdHG97, ηAGB var | WW95, case A | Mass cut changed |
| 3 | vdHG97, ηAGB var | WW95, case B + M92 pre-SN yields | Winds from Z = Z⊙ massive stars included |
| 4 | vdHG97, ηAGB var | K06, εHN = 0 | SNII yields changed |
| 5 | vdHG97, ηAGB var | K06, εHN = 1 | HN nucleosynthesis included |
| 6 | vdHG97, ηAGB var | K06, εHN = 1 + Geneva pre-SN yields, υini ≠ 0 | Stellar rotation included |
| 7 | vdHG97, ηAGB var | K06, εHN = 1 + Geneva pre-SN yields, υini = 0 | |
| 8 | vdHG97, ηAGB const | K06, εHN = 1 + Geneva pre-SN yields, υini ≠ 0 | Mass loss along the AGB changed |
| 9 | vdHG97, minimum HBB | K06, εHN = 1 + Geneva pre-SN yields, υini ≠ 0 | HBB extent reduced |
| 10 | M01, α = 1.68 | K06, εHN = 1 + Geneva pre-SN yields, υini ≠ 0 | LIMS yields changed |
| 11 | M01, α = 2.50 | K06, εHN = 1 + Geneva pre-SN yields, υini ≠ 0 | HBB strength increased |
| 12 | M01, α = 1.68 | K06, εHN = 1 + [Geneva, υini ≠ 0 + M92] pre-SN yields | |
| 13 | KL07, with extra pulses | K06, εHN = 1 + Geneva pre-SN yields, υini ≠ 0 | AGB yields from detailed stellar models |
| 14 | KL07, with extra pulses | K06, εHN = 1 + [Geneva, υini ≠ 0 + M92] pre-SN yields | |
| 15 | K10, without extra pulses | K06, εHN = 1 + Geneva pre-SN yields, υini ≠ 0 | Up-to-date nuclear reaction rates for LIMSs |
Notes. vdHG97: van den Hoek & Groenewegen (1997); WW95: Woosley & Weaver (1995); M92: Maeder (1992); K06: Kobayashi et al. (2006); M01: Marigo (2001); KL07: Karakas & Lattanzio (2007); K10: Karakas (2010). The models adopting the yields by Marigo (2001) for LIMSs use self-consistent nucleosynthesis prescriptions from Portinari et al. (1998) for stars of initial mass m = 6 M⊙ and m = 7 M⊙.
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