Mass 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 star||0.0||8.64 ×10-5|
|Herzsprung gap star||0.0||3.75 ×10-5|
|First giant branch star||9.95 ×10-5||4.40 ×10-5|
|Core He-burning star||0.0||1.49 ×10-4|
|Asymptotic giant branch star||0.0||2.87 ×10-5|
|He-star||1.42 ×10-3||4.96 ×10-3|
|He-giant star||1.46 ×10-1||2.02 ×10-1|
|Total, all types||1.48 ×10-1||2.08 ×10-1|
|τaccr [yr]||5.9 ×104||8.5 ×104|
|Naccr (1010LB, ⊙ galaxy)||1.8 ×102||2.5 ×102|
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