Notes. Surface trans-Fe abundances are from our Model D progenitor and are applied in the outermost ∼0.11 M_⊙. The adopted ²²Ne(α,n)²⁵Mg and ²²Ne(α,γ)²⁶Mg reaction rates are from Wiescher et al. (2023). The last column shows the final yields from the same explosive model but without the inclusion of trans-Fe element enrichment in the external layers of the primary WD, and with a ²²Ne abundance equal to the accreted value for model D (as specified in Table 1). The elemental ratios [Rb/Sr] and [Rb/Zr] are also given in square bracket notation in the last two lines.