Table 4.
Summary of the underlying model dependency for SNIa enrichment (Eq. (3)).
| Index | Model | Index | Model |
|---|---|---|---|
| 1 | CDD1 | 2 | CDD2 |
| 3 | W7 | 4 | W70 |
| 5 | WDD1 | 6 | WDD2 |
| 7 | WDD3 | 8 | DDTa |
| 9 | DDTb | 10 | DDTc |
| 11 | DDTd | 12 | DDTe |
| 13 | DDTf | 14 | CDEF |
| 15 | ODDT | 16 | CDDT |
Notes. The CDD (i.e. indices 1 and 2) and WDD (5–7) models are delayed-detonation scenario (Iwamoto et al. 1999). The W (3 and 4) models refer to convection deflagration scenario (Iwamoto et al. 1999). The DDT (8–12) models are based on observational results from the Tycho supernova remnant (Badenes et al. 2006). The CDEF model refers to 2D deflagration scenario, and the ODDT and CDDT models both refer to the 2D delayed-detonation scenario (Maeda et al. 2010).
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.