and its inverse which set the stationary abundances of the non-alpha-particle isotopes, where the free densities of protons and neutrons are also established by the quasiequilibrium. However, the abundance of free neutrons is also proportional to the excess of neutrons over protons in the composition of the massive star; therefore the abundance of Ar, using it as an example, is greater in ejecta from recent massive stars than it was from those in early stars of only H and He; therefore Cl, to which Ar decays after the nucleosynthesis, is called a "secondary isotope".