Average masses accreted by the first-formed WDs in DD progenitor systems in our sample that experience a combination of RLOF and wind mass transfer, split by donor type.
|Main sequence||0.0||1.04 ×10-4|
|Herzsprung gap||0.0||2.74 ×10-5|
|First giant branch||1.20 ×10-4||1.86 ×10-5|
|Core He-burning||0.0||3.12 ×10-4|
|Asymptotic giant branch||0.0||6.63 ×10-5|
|He-star||8.35 ×10-5||3.26 ×10-3|
|He-giant||1.43 ×10-1||2.01 ×10-1|
|Total, all types||1.43 ×10-1||2.05 ×10-1|
|τaccr [yr]||5.8 ×104||8.42 ×104|
|Naccr (1010LB, ⊙ galaxy)||1.7 ×102± 13||2.5 ×102± 16|
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