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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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