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- W4294328556 endingPage "A5" @default.
- W4294328556 startingPage "A5" @default.
- W4294328556 abstract "Aims. Recently, the study of globular cluster (GC) color−magnitude diagrams (CMDs) has shown that some of them harbor multiple populations with different chemical compositions and/or ages. In the first case, the most common candidate is a spread in the initial helium abundance, but this quantity is difficult to determine spectroscopically due to the fact that helium absorption lines are not present in cooler stars, whereas for hotter GC stars gravitational settling of helium becomes important. As a consequence, indirect methods to determine the initial helium abundance among populations are necessary. For that reason, in this series of papers, we investigate the effects of a helium enrichment in populations covering the range of GC metallicities." @default.
- W4294328556 created "2022-09-02" @default.
- W4294328556 creator A5021960779 @default.
- W4294328556 creator A5040528710 @default.
- W4294328556 creator A5066099281 @default.
- W4294328556 date "2012-10-18" @default.
- W4294328556 modified "2023-09-25" @default.
- W4294328556 title "Effects of helium enrichment in globular clusters" @default.
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