Table 1
White dwarf mass ranges in our simulation (S) and those for which cooling tracks are available in the literature (L).
| Z = 0.0001 | Z = 0.001 | Z = 0.004 | Z = 0.01 | Z = 0.02 | |
|
|
|||||
| He (S) | 0.144 | 0.161 | 0.148 | 0.146 | 0.142 |
| 0.509 | 0.496 | 0.487 | 0.481 | 0.476 | |
|
|
|||||
| CO (S) | 0.330 | 0.330 | 0.330 | 0.330 | 0.330 |
| 1.38 | 1.29 | 1.33 | 1.35 | 1.38 | |
|
|
|||||
| CO (L) | 0.520 | 0.505 | 0.503 | 0.525 | 0.54 |
| 0.826 | 0.863 | 0.817 | 0.934 | 1.20 | |
Notes. The mass range for He core WD cooling tracks that are available in the literature is 0.155−0.435 (only available for metallicity Z = 0.01). Magnitudes in the V and I band as a function of cooling time for He core WDs are only available for WDs in the mass range 0.220−0.521, whose progenitors have metallicity Z = 0.03. The mass range for ONe WD cooling tracks that is available in the literature is 1.06−1.28 (only available for metallicity Z = 0.02). The simulations yield ONe WDs in the mass range 1.10−1.38 (this simulated mass range is the same for all metallicities).
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