The efficiency of the slow neutron-capture process in massive stars is strongly influenced by reactions on light elements. At low metallicity, $^{16}$O an important neutron absorber, but effectiveness as a light-element poison modified competition between subsequent $^{17}$O$(\alpha,n)^{20}$Ne and $^{17}$O$(\alpha,\gamma)^{21}$Ne reactions. strengths key resonances within Gamow window for core ...