Table 2.
Resulting WD mass as a function of the initial mass Mini and rotation parameter value f for our computed models.
| Mini/M⊙ | f |
||||||
|---|---|---|---|---|---|---|---|
| 0 | 0.02 | 0.05 | 0.10 | 0.15 | 0.20 | 0.25 | |
| 4.0 | – | – | – | – | 0.82 | 0.93 | 0.98 |
| 5.0 | – | – | – | 1.02 |  |
 |
 |
| 5.5 | – | – | – |  |
 |
 |
 |
| 6.0 | 0.90 | – | – |  |
 |
 |
 |
| 7.0 | 0.97 | 1.01 |  |
 |
 |
 |
1.48 |
| 7.5 | 1.02 | 1.03 |  |
 |
 |
 |
– |
| 8.0 |  |
 |
 |
 |
 |
1.41 | 1.56 |
| 8.5 |  |
 |
 |
 |
 |
– | – |
| 9.0 |  |
 |
 |
1.40 | 1.48 | – | – |
| 9.5 |  |
 |
– | 1.41 | – | – | – |
Notes. Black, brown, blue, and italic numbers denote, respectively, the evolutionary outcome of normal CO, UMCO, ONe, and WDs with masses exceeding the Chandrasekhar mass value for non-rotating stars (see also Fig. 2).
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