Table 1
Characteristics of our initial He-core white dwarf models.
M f | P i | P f |
![]() |
M H | H flash |
(solar mass) | (days) | (days) | (solar mass) | ||
|
|||||
0.15540 | 0.90 | 0.23 | 0.365 | 4.34 × 10-3 | No |
0.16115 | 0.95 | 0.32 | 0.376 | 4.19 × 10-3 | No |
0.16499 | 1.0 | 0.35 | 0.390 | 4.09 × 10-3 | No |
0.17064 | 1.1 | 0.44 | 0.405 | 3.94 × 10-3 | No |
0.17624 | 1.2 | 0.54 | 0.423 | 3.80 × 10-3 | No |
0.18213 | 1.3 | 0.80 | 0.440 | 3.66 × 10-3 | Yes |
(0.18050) | |||||
0.18685 | 1.4 | 1.14 | 0.453 | 3.55 × 10-3 | Yes |
(0.18630) | |||||
0.19210 | 1.55 | 1.54 | 0.466 | 3.42 × 10-3 | Yes |
(0.19173) | |||||
0.20258 | 2 | 2.47 | 0.490 | 3.22 × 10-3 | Yes |
(0.20187) | |||||
0.23903 | 5.2 | 10.32 | 0.701 | 2.86 × 10-3 | Yes |
(0.23887) | |||||
0.27242 | 10 | 20.4 | 0.715 | 2.02 × 10-3 | Yes |
(0.27065) | |||||
0.32079 | 40 | 78.7 | 0.715 | 1.18 × 10-3 | Yes |
(0.32048) | |||||
0.36304 | 100 | 187.7 | 0.715 | 7.85 × 10-4 | Yes |
(0.36242) | |||||
0.43520 | 300 | 520 | 0.715 | 4.33 × 10-4 | No |
Notes. Mf: secondary mass at the end of Roche lobe overflow. Pi: initial orbital period of the system. Pf: final orbital period at the end of Roche lobe overflow. : hydrogen surface abundance at the end of Roche lobe overflow. MH: mass of the hydrogen content at the point of maximum effective temperature at the beginning of the first cooling branch. H flash: occurrence of CNO flashes on the early white dwarf cooling branch.
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