Mass accreted via wind mass transfer by the first-formed WDs in DD progenitor systems in our sample, split by donor type.
|Main sequence star||0.0||0.0|
|Herzsprung gap star||0.0||3.51 ×10-5|
|First giant branch star||0.0||4.37 ×10-5|
|Core He-burning star||0.0||2.28 ×10-6|
|Asymptotic giant branch star||0.0||1.86 ×10-6|
|He-giant star||0.0||3.00 ×10-3|
|Total, all types||0.0||4.07 ×10-3|
|τaccr [yr]||0.0||2.0 ×103|
|Naccr (1010LB, ⊙ galaxy)||none||6.0|
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