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- W1965432896 abstract "We explore the possibility that deep mixing is the reason that there are too many red giants in the Galactic globular clusters M5 and M30. Deep mixing has often been invoked to account for the abundance anomalies observed in many bright Galactic globular cluster giants. Here we assume that it also adds fuel to the hydrogen-burning shell of a typical giant in some clusters and returns helium to the envelope above. We use a simple mixing model to estimate how much extra fuel has been added to the hydrogen-burning shell of a typical red giant in M5 and M30 from the number of extra stars in the red giant branch (RGB) luminosity functions for these two clusters. Presumably, extra red giants are common in Galactic globular clusters. M5 and M30 were chosen solely because the available luminosity functions for both were derived from an exceptionally large sample of stars in two colors: the RGB luminosity functions are especially well defined and well normalized to unevolved main-sequence stars." @default.
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- W1965432896 date "2000-02-01" @default.
- W1965432896 modified "2023-09-24" @default.
- W1965432896 title "Globular Cluster Giant Branch Luminosity Functions: “Extra Stars” and “Deep Mixing”" @default.
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- W1965432896 doi "https://doi.org/10.1086/308283" @default.
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