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- W3103043790 abstract "Context. Long-lived stars in globular clusters exhibit chemical peculiarities with respect to their halo counterparts. In particular, sodium-enriched stars are identified as belonging to a second stellar population born from cluster material contaminated by the hydrogen-burning ashes of a first stellar population. Their presence and numbers in different locations of the colour-magnitude diagram provide important constraints on the self-enrichment scenarios. In particular, the ratio of Na-poor to Na-rich stars on the asymptotic giant branch (AGB) has recently been found to vary strongly from cluster to cluster (NGC 6752, 47 Tuc, and NGC 2808), while it is relatively constant on the red giant branch (RGB)." @default.
- W3103043790 created "2020-11-23" @default.
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- W3103043790 date "2016-01-21" @default.
- W3103043790 modified "2023-09-30" @default.
- W3103043790 title "Evolution of long-lived globular cluster stars" @default.
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- W3103043790 doi "https://doi.org/10.1051/0004-6361/201527576" @default.
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