Table 5
Properties of the last computed models with effective temperatures between 3.6 and 4.3 ordered from top to bottom by increasing effective temperatures (in logarithm).
T eff | L / L⊙ | Model | Mfin | M α | M CO |
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m H |
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|
||||||||
3.606 | 4.057 | 9/25/0.4 | 2.60 | 2.27 | 0.94 | 1.44 | 0.21 | 0.16 |
3.612 | 4.856 | 15/10/0 | 4.88 | 4.24 | 2.24 | 1.58 | 0.28 | 0.14 |
3.621 | 4.926 | 15/25/0.4 | 5.32 | 4.70 | 2.71 | 1.70 | 0.24 | 0.12 |
3.626 | 5.039 | 20/10/0 | 6.68 | 6.10 | 3.81 | 1.27 | 0.27 | 0.11 |
3.655 | 4.944 | 15/10/0.4 | 5.31 | 4.92 | 2.79 | 1.60 | 0.15 | 0.08 |
3.739 | 4.787 | 15/25/0 | 4.69 | 4.70 | 2.21 | 1.55 | 0.21 | 0.11 |
3.933 | 5.027 | 20/25/0 | 6.50 | 6.04 | 3.75 | 1.23 | 0.22 | 0.09 |
4.212 | 5.178 | 20/25/0.4 | 7.26 | 6.89 | 4.52 | 1.26 | 0.14 | 0.07 |
4.219 | 5.181 | 20/10/0.4 | 7.36 | 6.96 | 4.86 | 1.27 | 0.15 | 0.07 |
4.232 | 5.221 | 25/10/0 | 8.26 | 7.90 | 5.54 | 1.11 | 0.16 | 0.07 |
4.233 | 5.262 | 25/25/0 | 8.35 | 8.02 | 5.66 | 1.11 | 0.14 | 0.06 |
Notes. The luminosity is in logarithm, the masses in solar masses. The model nn/mm/pp corresponds to the models with an initial mass nn, a RSG mass-loss rate increased by a factor mm, and an initial rotation on the ZAMS equal to pp times the critical velocity υcrit.
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