Table 1.
Characteristics of our 25 M⊙, Z = 10−3 stellar models at the end of their evolution.
| Model label | υini/υcrit | 17O(α,γ)21Ne | MCO | MNi |
|---|---|---|---|---|
| [M⊙] | [M⊙] | |||
| M25Zm3V0 | 0 | Best et al. (2013) | 5.90 | 1.11 |
| M25Zm3V4 | 0.4 | Best et al. (2013) | 7.61 | 1.31 |
| M25Zm3V7 | 0.7 | Best et al. (2013) | 7.56 | – |
| M25Zm3V0B | 0 | Best et al. (2013)/10 | 5.88 | – |
| M25Zm3V4B | 0.4 | Best et al. (2013)/10 | 7.64 | – |
| M25Zm3V7B | 0.7 | Best et al. (2013)/10 | 7.62 | – |
| M25Zm3V0C | 0 | Taggart et al. (2019) | 5.88 | – |
| M25Zm3V4C | 0.4 | Taggart et al. (2019) | 7.65 | – |
| M25Zm3V7C | 0.7 | Taggart et al. (2019) | 7.57 | – |
Notes. MCO (Col. 6) is the mass of the carbon-oxygen core, defined where the mass fraction of 4He has dropped below 10−2. MNi (Col. 7) is the mass of the Ni core, defined when the mass fraction of 56Ni drops below 10−2 (the models without a value for MNi were not computed until the very end of the evolution; see text for details).
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.