New theoretical yields of intermediate mass stars

Bob van den Hoek, Martin Groenewegen

We present theoretical yields of H, ${}^4$He, ${}^{12}$C, ${}^{13}$C, ${}^{14}$N, and ${}^{16}$O for stars with initial masses between 0.8 and 8 M${}_{\odot }$ and initial metallicities Z = 0…