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Table A.1.
Adopted stellar and binary evolution parameters in MESA.
| Parameter | Value |
|---|---|
| initial post-CE orbital period | 2.5, |
| initial post-CE white dwarf mass | 0.6, 0.7, 0.8, 0.9, 1.0 M⊙ |
| initial post-CE companion mass | 1.0, 1.1, 1.2, 1.3, 1.4, 1.5 M⊙ |
| Metallicity Z | |
| criterion for stable H shell burning | Wolf et al. (2013) |
| MB prescription | CARB (Van & Ivanova 2019) |
| CAML prescription | mass loss (King & Kolb 1995) |
| Reimers’s parameter | 0.5 |
| MLT | Henyey et al. (1965) |
| mixing length (Hp) | 1.5, 2.0, 2.5 |
| extent of diffusive | 0.016 Hp |
| exponential core overshooting | |
| criterion for stability | Schwarzschild (∇ad = ∇rad) |
| against convection | |
| opacity | Ferguson et al. (2005), |
| Freedman et al. (2008, 2014) | |
| nuclear network | cno_extras.net |
| atmosphere boundary conditions | Eddington T(tau) relation |
| how opacities are calculated | varying, iterated |
| throughout the atmosphere |
Notes. When more than one value of the parameter is varied in the search, the values adopted for the best-fitting models (i.e. Table 2) are highlighted in boldface (magenta for V1082 Sgr, green for V479 And, and black for both).
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