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Table A.1.
Parameter definitions for tables A.2 and A.3
| Parameter | Unit | Definition |
|---|---|---|
| Mi | (M⊙) | Initial total ZAMS mass |
| Ma | (M⊙) | Total mass after the end of mass-transfer, when the nuclear helium-burning luminosity exceeds 85% of the nuclear luminosity |
| Mb | (M⊙) | Total mass at core helium depletion, when the mass fraction of helium reaches values smaller than 10−4 |
| Mf | (M⊙) | Total mass at the end of the simulation when the mass fraction of carbon drops below 10−4 |
 |
(M⊙) | Mass of the carbon/oxygen core at the end of the simulation |
 |
(10−2 M⊙) | Total hydrogen mass after the end of mass-transfer |
 |
(10−2 M⊙) | Total hydrogen mass at the end of the simulation |
| Rmin | (R⊙) | Minimum radius |
| Rb | (R⊙) | Radius at core helium depletion |
| Rp | (R⊙) | For low-metallicity models, radius at the peak of the first radius expansion |
| Δtp | (kyr) | For low-metallicity models, difference between the final stellar age and the time of the peak of the first radius expansion |
| RC ign. | (R⊙) | Radius at core carbon ignition, when the luminosity of carbon exceeds 98% of the nuclear luminosity |
| Rmax | (R⊙) | Maximum radius |
| Rf | (R⊙) | Radius at the end of the simulation |
 |
(K) | Effective temperature at the end of the simulation |
| Lf | (L⊙) | Luminosity at the end of the simulation |
| gf | (cm s−2) | Surface gravity at the end of the simulation |
| Sf | Approximate final stellar type derived based on the effective temperature (see Sect. 4.1) |
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