Published online by Cambridge University Press: 25 March 2006
We present a summary of the extensive problems posed by the curious abundance correlations seen in stars in Galactic globular clusters.We discuss three scenarios, and conclude that only one seems to beconsistent with the observations. Even this is still rather unsatisfyingfrom many viewpoints. We determine the kind of nucleosynthesis requiredand discuss AGB stars as the possible source. Some calculations seem torule out AGB stars and others seem to favour them. The reasons for the differences are discussed. No satisfying conclusion is reached!