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- W1631047522 abstract "Evidence for non-homogeneity in the metal abundances of giant stars in various globular clusters is reviewed. The nonhomogeneity is of two kinds: (1) differences in the value of from star to star in the same cluster, for particular values of A, and (2) non-constancy of the cluster mean value of as a function of A. Observational evidence for the existence of variations of both kinds is cited, and discussed for four “nucleosynthetic” groups of elements: viz ., s-process, Fe-peak, α-process, and CNO. The rival hypotheses of core-envelope mixing and primordial abundance variations are examined in the light of the observations." @default.
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- W1631047522 date "1978-01-01" @default.
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- W1631047522 title "Evidence for Non-Homogeneity in the Metal Abundances of Stars in Globular Clusters" @default.
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- W1631047522 doi "https://doi.org/10.1017/s0074180900145474" @default.
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