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Constraints on the distance moduli, helium and metal abundances, and ages of globular clusters from their RR Lyrae and non-variable horizontal-branch stars. I. M3, M15, and M92

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Description scientific article published in January 2016
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Publication date 2016
Language English
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https://archive.org/details/arxiv-1607.02088

https://iopscience.iop.org/article/10.3847/0004-637X/827/1/2/pdf

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