Astrophys.J. 149, 577 (1967)

R.L.Macklin, J.H.Gibbons

Quantitative test of s-process in stellar nucleosynthesis for solar system material

NUCLEAR REACTIONS ^{116,117,118,119,120}Sn, ^{144,147,148,149,150,152,154}Sm, ^86,87,88Sr, ^{90,91,92,94,96}Zr, ^{122,123,124,125,126,128,130}Te(n, γ), E=30 keV; measured reaction products, Eγ, Iγ; deduced σ, Maxwellian-averaged σ and their uncertainties.