On the He burning phases of the Carina dSph
classification
🌌 astro-ph.SR
keywords
burningcarinaphasesabundanceagreementalphaassumingchemical
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We performed a detailed comparison between predicted He burning phases and multiband photometry of the Carina dwarf spheroidal galaxy. We found a good agreement with the predictions computed assuming an {\alpha}-enhanced chemical mixture, indicating a mean metallicity [Fe/H] ~ -1.8 with a raw observed peak-to-peak spread in iron abundance of 0.4\pm0.2 dex.
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