Table 1.
Classification of binary-stripped and accretor star models based on the mass transfer history.
| MT class | Timing of hydrogen-rich envelope removal |
|---|---|
| Single | None |
| Case A | During MS |
| Case Be | Between TAMS and TACHeB, radiative envelope |
| Case Bl | Between TAMS and TACHeB, convective envelope |
| Case C | After TACHeB |
Notes. Case A binary stripping or mass accretion takes place during the MS evolution of the donor and accretor, respectively, Case B between the TAMS and terminal age core helium burning (TACHeB) and Case C after TACHeB. Early and late Case B (Be/Bl) are stars with a radiative and mostly convective envelope, respectively.
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