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Table 2
Cooling times, in Gyr, at log (L/⊙) = −4.0 for different values of Ġ/G and two representative white dwarf masses.
| Ġ/G | MWD/M⊙ | |
|
|
||
| 0.609 | 1.0 | |
|
|
||
| 0 | 5.200 | 7.798 |
| −1 × 10-12 | 5.148 | 7.502 |
| −1 × 10-11 | 4.677 | 6.718 |
| −5 × 10-11 | 3.435 | 3.311 |
Notes. For these cooling sequences the present value of G occurs at this value of the stellar luminosity.
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